The galaxy presents as an elliptical morphology, appearing largely smooth and centrally concentrated with a high degree of radial symmetry. A dominant, concentrated bulge is observed, with a distinct decrease in luminosity moving outward. There is no apparent spiral arm structure, dust lanes, or significant star-forming regions visible. The galaxy exhibits a yellowish-red color, indicative of an older stellar population. The light profile suggests a significant population of evolved stars, likely resulting in low levels of current star formation. The overall structure appears relatively undisturbed. There is a slight asymmetry in the outer regions, which may suggest minor gravitational interaction, however there is no clear indication of a major merger or tidal disruption. 
