The galaxy appears as a relatively compact, disk-like structure. Its color profile suggests a range of stellar populations, with a bright, centrally concentrated region possibly indicating an older population or a bulge. A surrounding disk-like structure shows hints of spiral arms. There seems to be some form of a disturbance in the symmetry of the galaxy, potentially indicating minor interactions or tidal effects. There are hints of gas clouds towards the outer edges of the galaxy, which suggest active regions of star formation. The overall color profile indicates that star formation is happening in the arms, but that the bulk of the galaxy is older stars.
