The galaxy presents as a centrally concentrated system with a largely smooth, elliptical morphology. Its core exhibits a bright, compact region that diminishes gradually outward. Color gradients are subtle but noticeable, with the central region appearing slightly redder, transitioning to a greener hue in the outer regions. There is little evidence of spiral arm structure or significant dust lanes, suggesting a relatively passive star formation history. The galaxy appears undisturbed, showing no strong signs of tidal interactions or recent merger events.
