The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth light profile, with no discernible spiral arms or distinct features typically associated with disk galaxies. The core region appears brighter and slightly yellowish, suggesting an older stellar population. There is no clear dust lane or significant morphological disturbance, hinting that the galaxy is relatively undisturbed. Its overall shape is roughly round. The galaxy demonstrates no signs of recent major merger events, although minor disturbances or interactions cannot be ruled out.
