The galaxy presents a primarily smooth morphology. It appears elliptical in shape, exhibiting a radial concentration of light towards a bright, unresolved central region. The color profile suggests a primarily older stellar population, with a yellowish-white hue dominating the core and inner regions. Fainter, bluer light surrounds the core and inner regions of the galaxy, which is consistent with a small level of on-going star formation. There are no apparent signs of spiral arms or a bar structure. The galaxy's outer edges fade gradually into the background, indicating a diffuse halo. No significant tidal features or close companion galaxies are visible, suggesting that it is not undergoing a major merger event. The overall impression is that of a relatively evolved and quiescent system.
