The galaxy presents as a somewhat elongated, elliptical-like structure. It exhibits a smooth, centrally concentrated light distribution, suggesting a dominant bulge component. The galaxy's color is predominantly reddish-yellow, indicative of an older stellar population with lower levels of current star formation. There may be some degree of interaction or tidal disturbance evidenced by a minor asymmetry in the outer regions of the galaxy. This is possibly due to a minor merging event, the effects of which are still visible on the galaxy’s structure.
