The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity extending outwards from the core. The overall shape is roughly round. There is subtle evidence of a slight bluer color in the central region compared to the outer parts, suggesting potentially younger stellar populations and ongoing, but low, star formation. There are no apparent spiral arm structures or significant dust lanes visible within the galaxy's disk. No major mergers or tidal disturbances are observed, with only slight irregularities in the outer regions.
