The galaxy appears to be a relatively smooth, centrally concentrated object, exhibiting a predominantly elliptical morphology. The central region is bright and slightly reddish, suggesting a population of older stars. Surrounding the core is a fainter, more diffuse halo with a bluish tinge, perhaps indicating some ongoing, albeit limited, star formation. The galaxy appears largely undisturbed, with no signs of major mergers or tidal features. The overall structure suggests a relatively evolved galaxy with a dominant spheroidal component.
