The galaxy appears to be a relatively smooth elliptical or lenticular type. It displays a centrally concentrated luminosity profile, with a gradual decrease in surface brightness towards the outer regions. The core is bright and somewhat compact. The overall shape of the galaxy appears fairly regular with the shape being between round and cigar-shaped. There is no obvious sign of spiral arms or a prominent disk structure. The light distribution suggests that it is largely composed of older stellar populations. There are no distinct signs of star formation regions. The color indices imply a population of older stars, which is consistent with a relatively low star formation rate. There are no signs of active galactic nuclei.
