The galaxy presents as a relatively smooth, centrally concentrated object. It appears roughly elliptical in shape, displaying a gradual decrease in luminosity from the core outwards. The central region exhibits a yellowish-white hue, potentially indicative of an older stellar population. The outer regions show a bluer tint, suggesting some ongoing star formation, albeit at a seemingly low rate. There is no discernible spiral structure or bar. A slight asymmetry is present, with a subtle extension visible on one side. This could be a faint tidal feature hinting at a past interaction, but it could also simply be an irregular distribution of stars and gas. There's no obvious indication of an active galactic nucleus based on this image alone.
