The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated central bulge which appears more luminous than the surrounding halo. The light distribution suggests a near-spherical shape, though there may be a slight elongation along one axis. There is a very slight hint of distortion in the halo, indicating a possible minor gravitational interaction, but no obvious tidal tails or other signs of a major merger event are visible. The color suggests an older stellar population and low star formation rate. The overall morphology is consistent with an early-type galaxy.
