The galaxy presents as a centrally concentrated object, with a mostly smooth light distribution. The core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Moving outwards from the central region, the light profile fades gently into a more diffuse halo. The galaxy displays a slightly elliptical morphology, with minimal evidence of spiral arms or distinct features. There are no obvious signs of ongoing mergers or tidal disturbances. The galaxy's overall smooth and concentrated appearance suggests it is likely an early-type galaxy.
