The galaxy presents as a relatively compact object with a smooth, centrally concentrated light profile. There is a slight elongation in its morphology, but overall the shape appears mostly spheroidal. Color gradients across the galaxy are subtle. The central region appears somewhat yellower than the outer edges, suggesting a population of older stars. There is faint indication of asymmetry or minor perturbation in the outer halo but overall there are no signs of major ongoing interactions or merging events. It has a considerable mass and appears to have relatively low star formation.
