The galaxy presents as a luminous elliptical, with a smooth, centrally concentrated morphology. The core region exhibits a bright, golden hue indicative of an older stellar population. The outer regions of the galaxy fade gradually into a less defined halo, showing a slight elongation along its major axis. Some subtle features or disturbances can be observed; particularly the presence of faint plumes extending outward from the central region, possibly indicative of past minor merger events. The overall color gradient suggests a red-sequence galaxy.