The galaxy presents as a relatively smooth, centrally concentrated structure, with a largely spheroidal morphology. It exhibits a yellowish-red hue across its entirety, suggesting an older stellar population and a reduced rate of ongoing star formation. There is a slight deviation from perfect circularity, appearing somewhat elliptical. There are also other objects in proximity to this galaxy that might be exhibiting tidal features, which may suggest a possibility of interaction or merging events. These interactions may explain a slightly disturbed morphology.
