The galaxy presents a largely smooth and elliptical morphology. It exhibits a bright, concentrated core region that gradually fades into a more diffuse outer halo. The core appears to be yellowish-white. There may be slight disturbances to the arms with a possibility of other galactic mergers but the effects on the morphology are minor. The overall shape of the galaxy is mostly round, with a slight tendency towards being in between round and cigar shaped. There is some evidence of ongoing star formation activity, although at a relatively low rate as indicated by the redder color. The color gradient suggests a population of older stars dominating the central regions, with some younger, bluer stars residing in the outer regions of the galaxy.