The galaxy presents as an elliptical morphology, with a high degree of smoothness. It exhibits a concentrated, bright central bulge that graduates outward into a more diffuse halo. The overall shape appears somewhat rounded, with no prominent disk-like structures visible. A subtle color gradient is present, with the central region appearing more yellow, potentially indicative of an older stellar population. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed.
