The galaxy presents as an elliptical or lenticular structure. It exhibits a centrally concentrated luminosity profile, characterized by a bright, yellowish core that likely hosts an older stellar population. There is a relatively smooth transition from the bright core to the outer regions of the galaxy. The outer regions of the galaxy are more diffuse and have a bluer tinge. There is no indication of a prominent disk or spiral arms, nor signs of a major merger event disrupting the overall morphology. There is only a slight disturbance to the smoothness of the galaxy.
