The galaxy presents an elliptical morphology, with a smooth, concentrated light profile that suggests an older stellar population. The galaxy exhibits a significant central bulge that transitions into a fainter, more diffuse halo. The overall color is moderately red, indicating the presence of evolved stars and a reduced rate of ongoing star formation.

There is evidence of some disk-like features or disturbances in the galaxy's outer regions. The disturbance could be indicative of a possible ongoing or recent minor merger event. Further observations are needed to determine whether these are tidal features or intrinsic structural components.