The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular system. It exhibits a slightly elongated morphology, with the primary axis extending horizontally in the image. A distinct, bright core region is observable. The galaxy displays a general yellow-white hue, indicative of a population of older stars. There are no clear signs of spiral arm structures or significant dust lanes. Faint traces of light extend from the core region into a diffuse halo, showing a gradual decrease in surface brightness with increasing radial distance. No signs of tidal disturbances or interactions with other galaxies are readily visible. Overall, the galaxy appears to be a mature system.
