The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse morphology. The central region exhibits a strong, yellowish luminosity, indicating an older stellar population. The overall shape is noticeably elongated, but lacks the clear features of a spiral or barred spiral galaxy. There is a faint, diffuse halo surrounding the core, with a slight decrease in intensity away from the center. There is a hint of bluer color on one side of the halo, suggesting the possibility of some star formation in the outer regions, but overall, the galaxy appears to be dominated by an evolved stellar population. Minor disturbances in the symmetry of the outer halo are present, however no obvious merging events can be observed.
