The galaxy appears to be an elliptical galaxy, as evidenced by its smooth and featureless morphology. It exhibits a cigar-like shape, with a noticeable elongation along one axis. The light distribution suggests a centrally concentrated stellar population, with a gradual decrease in luminosity towards the outer regions. The color profile indicates an older stellar population, with a yellow-red hue dominating the central bulge. The outer regions display a bluer tint, potentially indicating a minor presence of younger stars or star-forming regions. There is no apparent spiral structure or dust lanes visible. No signs of major mergers or significant tidal disturbances are observed; however, a very slight asymmetry could indicate a minor past interaction. The overall impression is that of a relatively evolved and quiescent galaxy.
