The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile with a gradual decline in intensity outwards from the core. There is little evidence of spiral arms, bar structures, or significant dust lanes. The galaxy appears relatively round in shape. A subtle color gradient is observed, with the central region exhibiting a slightly bluer hue compared to the outer regions, which appear redder. This may be due to a slightly larger concentration of younger stars in the core of the galaxy. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
