The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical or lenticular, lacking a prominent spiral arm structure. There is a slight elongation to the galaxy's shape; it is not perfectly circular. The color profile exhibits a yellowish-red hue, suggestive of an older stellar population and limited ongoing star formation. The object's smooth appearance is coupled with only minor disturbances, which likely indicates it has not undergone a major merger event recently. The galaxy has a medium mass and a corresponding low star formation rate.
