The galaxy appears as a centrally concentrated object with a smooth, diffuse halo. The core region displays a relatively high surface brightness. The overall morphology suggests an elliptical or lenticular galaxy, with a somewhat rounded appearance. There is a subtle elongation along one axis, but no clear spiral arm structure or prominent dust lanes are evident. There may be a slight tidal disturbance. Its red color indicates a significant population of older stars. There is no evidence of strong, ongoing star formation.
