This galaxy exhibits a relatively smooth and rounded morphology. There is a discernible lack of spiral arm structure or a prominent disk component. The galaxy presents as generally elliptical, though not perfectly spherical, with a minor elongation. Color gradients suggest a redder core region which indicates a greater population of older stars. The galaxy does not show any signs of major disturbances due to recent or ongoing mergers, although minor disturbances cannot be ruled out definitively.
