The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. Its light profile suggests a dominant spheroidal component, lacking distinct spiral arm structures or a prominent galactic disk. The color index, inferred from the redder central region transitioning to slightly bluer outer edges, implies a likely evolved stellar population in the core. There's a hint of extended halo, but of generally low surface brightness. No indications of recent major mergers or strong tidal disturbances are evident.
