The galaxy presents as a single, somewhat diffuse object. It is roughly elliptical in shape, with a smooth, centrally concentrated luminosity profile. The core region exhibits a yellow-orange hue, suggestive of an older stellar population. The outer regions appear fainter, with a slight transition towards a bluer color, indicating the possible presence of some younger stars, but they are not particularly distinct. There is no obvious spiral structure, bar, or significant dust lane visible. No major disturbances or indications of ongoing or recent merger activity are readily apparent in the morphology of this galaxy.
