The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light profile. The core region is luminous and appears yellowish, likely indicating a population of older stars. The outer regions display a more diffuse, bluer hue. The galaxy appears to be a relatively isolated system, without obvious signs of major ongoing mergers. However, there is faint structure suggesting possible minor disturbance on one side. The disk is relatively small compared to other galaxies. Overall, it appears to be a moderate sized galaxy at an intermediate distance.
