The Sombrero Galaxy, M104, as seen by Spitzer, JWST, and Hubble.
Notice the outer ring, which appears smooth in the lower-resolution Spitzer image, shows glowing clumps of dust in the mid-infrared JWST image. These same dusty clumps appear dark in the visible light Hubble image.
The dust JWST sees is made of soot-like carbon-containing molecules called polycyclic aromatic hydrocarbons. They can indicate the presence of young star-forming regions.
More: https://webbtelescope.org/contents/news-releases/2024/news-2024-137