The galaxy presents as a relatively smooth, elliptical-like structure. A concentrated, bright central bulge dominates the galaxy's overall morphology. Fainter, extended emission surrounds the central bulge, fading into the background. There is minimal evidence of spiral arm structures or prominent dust lanes within the galaxy. The color appears yellowish, potentially indicating an older stellar population. The galaxy does not appear to be undergoing any major mergers or tidal disturbances based on the symmetry and lack of extended tidal tails. Overall, the galaxy seems to be a relaxed, relatively undisturbed system dominated by older stars.
