The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is no apparent spiral structure or prominent dust lanes. The core region displays a yellowish-white hue, potentially indicative of an older stellar population. Moving outward from the center, the light becomes less intense, transitioning to a bluish-white coloration. This color gradient suggests a possible distribution of younger stars in the outer regions, however, star formation is low overall. The galaxy is largely undisturbed, with no obvious signs of recent major merger events.
