The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The light distribution appears centrally peaked. There is a clear, diffuse halo surrounding the main body of the galaxy, extending outwards. While a distinct disk is not readily apparent, there might be a very faint, diffuse disk component. The color profile suggests that the galaxy is likely composed of an older stellar population, indicative of limited ongoing star formation, consistent with an early-type galaxy classification. Based on visual assessment, there are no obvious signs of tidal features or major disturbances indicative of recent merger activity.
