The galaxy presents as a somewhat elongated, elliptical shape. It exhibits a smooth, centrally concentrated light profile, with a gradual decrease in luminosity outwards from the core. The core is a bright, yellow hue, likely indicating a population of older stars. Moving outwards, the galaxy displays a more orange tint, potentially indicating a mix of stellar populations. There is some indication of possible slight distortions in the outer regions, which may suggest tidal interactions or past minor mergers. Star formation appears relatively quiescent.
