The galaxy presents a centrally concentrated, elliptical morphology. The core exhibits a bright, yellowish-white luminosity, indicative of an older stellar population. There is a moderate color gradient extending outwards from the core, transitioning into a more diffuse, somewhat bluer halo. This suggests the presence of a younger stellar population in the outer regions, but is not particularly pronounced. The overall structure appears relatively undisturbed, showing no obvious signs of recent major mergers, although there is some minor asymmetry. The smoothness of the light distribution suggests it is likely an early-type galaxy with a relatively low star formation rate. The galaxy is approximately 8 kpc in radius.