The galaxy presents a smooth, elliptical morphology with a centrally concentrated, bright bulge. The galaxy appears quite round, exhibiting little to no disk-like structure or spiral arms. The light from the galaxy is reddish-orange, implying a population of older stars and a relatively low rate of ongoing star formation. There are indications of a potential minor disturbance of structure but the central concentration remains compact and there is no major disturbance or clear merger event readily apparent. The galaxy's overall structure indicates it is a massive system.
