The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is generally elliptical, appearing somewhat rounded rather than highly elongated. There is a distinct color gradient noticeable, with the central region exhibiting a more yellowish-orange hue that transitions towards a slightly bluer periphery. Evidence of spiral arms or distinct dust lanes is lacking. Based on its morphology, the galaxy appears to be in a relatively quiescent state, showing little evidence of major ongoing mergers or significant disturbances. It exhibits a moderate level of star formation activity, consistent with a population of older stars dominating the central region while younger stars contribute to the bluer outer regions.
