The galaxy appears as a generally smooth, elliptical-shaped object. It displays a concentrated central bulge that is bright white. The light tapers off moving outwards from the central bulge. The galaxy exhibits a bluer hue overall. There's no significant dust lane or spiral arm structure visible. The outer edges fade gradually into the background sky, suggesting a diffuse halo or extended stellar population. There is no evidence of a recent major merger. Minor disturbances are possible.
