The galaxy presents a generally elliptical morphology, though not perfectly so. It exhibits a smooth, featureless appearance, lacking the spiral arms or prominent dust lanes often seen in other galaxy types. The light distribution is centrally concentrated, with a bright core that gradually fades towards the outer edges. There is a slight elongation. The color profile suggests a population of older stars, as indicated by the reddish-yellow hue dominating the central region. The outer regions appear somewhat bluer, possibly indicating some younger stellar populations. There is no obvious signs of on-going major mergers. Minor disturbances are possible.
