The galaxy presents as an elliptical or lenticular morphology, exhibiting a generally smooth and centrally concentrated light distribution. There is a noticeable lack of spiral arm structure. It exhibits a yellowish-orange hue, indicative of an older stellar population and reduced ongoing star formation activity. The galaxy appears to be a part of a pair of galaxies, in which one is a smoother morphology than the other. There is faint surrounding structure, perhaps suggesting the presence of tidal features or a diffuse halo.
