The galaxy presents as an elliptical morphology, appearing relatively smooth with a concentrated central bulge. The light distribution suggests an older stellar population, based on the redder hue dominating the galactic body. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat elongated. There is a hint of possible tidal interaction or minor disturbance in the outer regions, though the main structure appears largely undisturbed. The overall impression is of a mature, relatively quiescent galaxy.
