This galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that is bright and yellowish-white in color, indicating an older stellar population. The outer regions show a gradual decrease in surface brightness, transitioning to a fainter, more diffuse halo. There is very little evidence of spiral arm structure or significant dust lanes, suggesting it is a quiescent system with a low rate of star formation. The galaxy's overall shape is somewhat round, with a slight elongation along one axis. There are no obvious signs of tidal disturbances or ongoing mergers, implying it is a relatively isolated and undisturbed system.
