The galaxy presents as an elliptical morphology. It exhibits a bright, concentrated central bulge that appears largely spheroidal in shape. The color of the bulge is yellowish, likely indicating a population of older stars. There is an extended, diffuse halo surrounding the bulge. The outer regions of the galaxy show a gradual decrease in surface brightness with increasing radial distance. The halo also seems to have slightly bluer colors in the outer regions, indicative of a younger, bluer stellar population in comparison to the bulge. The galaxy appears relatively undisturbed, with no obvious signs of recent mergers or tidal interactions.
