The galaxy presents an elliptical morphology, appearing moderately smooth with a concentrated central bulge. A diffuse halo surrounds the central region, extending outwards. There is a slight distortion in the overall shape, possibly indicating a minor gravitational interaction or internal disturbances. Patches of bluer light are observed in a few regions on the periphery, which may indicate some ongoing star formation. The galaxy exhibits a dominant reddish-orange hue, suggesting an older stellar population is dominating the overall light output. There are traces of disturbances or tidal features, that might be suggestive of an ongoing or recent merger event.
