The galaxy presents as a centrally concentrated object, generally elliptical in shape, with a smooth, diffuse light profile. The core region exhibits a yellowish hue, suggestive of an older stellar population and a relatively low rate of recent star formation. There is very little discernible internal structure such as spiral arms or dust lanes. Overall, this galaxy appears to be relatively undisturbed, exhibiting a morphology consistent with a passively evolving system. Its apparent size is compact, with no evidence of major mergers or significant tidal interactions.
