The galaxy presents a generally elliptical morphology, appearing quite smooth and centrally concentrated. The core is bright, with a yellow-orange hue, indicating a population of older stars. This core smoothly transitions to a less luminous outer region. There is a blue region extending away from the central galaxy, but it is not clear if that is actually part of the galaxy. The overall structure suggests a system that has undergone significant dynamical relaxation, potentially a relatively quiescent galaxy with ongoing but low levels of star formation. Evidence for strong disturbances or tidal features is absent.
