The galaxy presents as a relatively smooth object with a primarily elliptical morphology. It exhibits a yellowish-red hue, suggestive of an older stellar population and comparatively low levels of ongoing star formation. The galaxy is largely spheroidal in shape and has high central stellar mass. There is evidence of possible merger activity or tidal disturbances in the asymmetry of the outer edges of the galaxy. This is further supported by its proximity to other objects in the image.
