The galaxy presents an elliptical morphology, appearing somewhat smooth and centrally concentrated. The luminosity profile indicates a gradual decline in brightness from the core outwards. The color appears generally redder, with a hint of a blue shift. The shape is closer to a sphere than a disk. The overall structure appears relatively undisturbed, lacking obvious signs of major merger activity. The color suggests the galaxy may be populated predominantly by older stars and have lower star formation rate. 
