The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The core region is bright and appears yellowish-white, suggesting a population of older stars. There is a gradual decrease in luminosity outwards from the center with no distinct spiral arm structure visible. The galaxy is elongated and moderately rounded in shape, showing no strong signs of recent or major merger activity. Faint hints of a disk-like structure may exist but is otherwise unconfirmed. Overall, the galaxy appears to be a relatively undisturbed and evolved system. 
