The galaxy presents as a spheroid, with a smooth, centrally concentrated light distribution. It exhibits a color gradient, appearing bluer in the outer regions and redder toward the core. There is some evidence of a possible tidal disturbance to the left of the central region of the spheroid. The galaxy is relatively compact. Overall, the galaxy appears to be a relatively massive early-type galaxy with an aging stellar population and subdued star formation, showing signs of potential recent or ongoing interaction or disturbance.
