The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. It exhibits a generally round morphology. There are faint, extended regions of diffuse light surrounding the central region. The galaxy's color profile indicates a population of older stars, with a reddish-yellow hue dominating the central bulge, fading to a slightly bluer color in the outer regions, implying ongoing, but diminished, star formation. There is little indication of spiral arm structure or significant dust lanes. There are no clear signs of major ongoing mergers or significant tidal disturbances, although faint asymmetry in the outer regions might suggest a past interaction.