The galaxy presents a morphology characterized by a dominant, centralized spheroid component. The overall color of the galaxy is yellowish, suggesting a relatively older stellar population. Evidences of ongoing or recent star formation are present, with a slightly bluer hue observed in the outer regions and in several faint knot-like features. These might signify regions of ionized gas around hot, young stars. The galaxy appears somewhat disturbed. There is a tidal tail or plume feature extending from the main body, possibly resulting from a gravitational interaction. The bulk of the galaxy looks fairly smooth, with the outer reaches being more disturbed. This galaxy is undergoing some sort of interaction.
