The galaxy presents as a somewhat diffuse, elliptical morphology. It exhibits a smooth appearance with a concentrated central bulge and a gradual decrease in luminosity towards its outer regions. There is a slight asymmetry in the light distribution, with a subtle extension of the galactic halo on one side, but no obvious signs of strong tidal interactions or major mergers. The color profile suggests a population of older stars dominating the central bulge, indicated by the yellowish hue. The outer regions appear slightly bluer, possibly signifying the presence of younger stellar populations or a minor amount of on-going star formation, although this is not pronounced. There is no distinct dust lane or spiral arm structure visible. The overall impression is that of a galaxy in a relatively quiescent state, characterized by a high mass and low star formation rate.
