The James Webb Space Telescope gives us a breathtaking intergalactic glimpse of life 32 million light-years from earth.

“Delicate gray, webby filaments form a spiral pattern winding outwards from the center of the galaxy. These spiral arms of the galaxy are traced by blue and bursts of pink; these are the regions in which stars are forming. The very heart of the galaxy is colored blue and has speckles, which are young stars, which are forming around the nucleus of the galaxy.” (Image credit: ESA/Webb, NASA & CSA, J. Lee and the PHANGS-JWST Team. Acknowledgement: J. Schmidt)
This image shows Webb near-infrared data combined with optical data from Hubble. Lacy red filaments spiraling out of the center of the galaxy are overlaid over a black field speckled with stars. The center of the galaxy glows in a pale color. The red filaments contain pops of bright pink, and some blue stars are visible in the background. The red color is dust, lighter oranges in the dust mean that dust is hotter. The young stars sprinkled through the arms and around the core of the galaxy are blue. Heavier older stars nearer the center of the galaxy are cyan and green and contribute to its glow. The pink pops of color are star forming regions. (Image credit: ESA/Webb, NASA & CSA, J. Lee and the PHANGS-JWST Team; ESA/Hubble & NASA, R. Chandar Acknowledgement: J. Schmidt)
“The Phantom Galaxy (M74) has been imaged in infrared and optical light using the James Webb Space Telescope and Hubble Space Telescope. The spiral galaxy is about 32 million light-years from Earth.” (VideoFromSpace)
“This image is divided evenly into 3 different views of the same region in the Phantom Galaxy. At left is an optical view taken by Hubble. Arms carved of brown filaments spiral out from a bright galactic core. The arms have pops of pink, which are star-forming regions, and there are blue stars throughout. The middle view contained combined Webb and Hubble data. Lacy red filaments spiraling out of the center of the galaxy are overlaid over a black field speckled with tiny blue stars. The red filaments contain pops of bright pink, which are star-forming regions. Lighter oranges in the red dust mean that dust is hotter. Heavier older stars closer to the center of the galaxy are cyan and green, and contribute to a greenish glow at the core. At right is a mid-infrared image from Webb. Delicate gray filaments spiral outwards from the center. These arms are traced by blue and bursts of pink, which are star-forming regions. A cluster of young stars glow blue at the very heart of the galaxy. (Image credits: ESA/Webb, NASA & CSA, J. Lee and the PHANGS-JWST Team. Acknowledgement: J. Schmidt)