The galaxy appears to be a relatively smooth, elliptical shape. The light distribution suggests a central bulge that dominates the luminosity profile, with a gradual decrease in surface brightness towards the outer regions. The galaxy exhibits a moderate degree of ellipticity. The galaxy's color appears somewhat redder in the central regions, transitioning to bluer hues in the outer areas, possibly indicating older stellar populations concentrated in the center and younger stars forming in the outer regions. There appears to be a slight disturbance or tidal feature on one side of the galaxy, hinting at a possible past interaction or minor merger. Overall, the galaxy seems to be a fairly mature system, but not without some ongoing activity.