The galaxy presents as a largely featureless, elliptical-like structure. It exhibits a smooth, concentrated light profile with a bright central core that fades gradually into a diffuse halo. The overall color appears relatively uniform, with a subtle gradient from a slightly redder center to a bluer outer region. No distinct spiral arms or prominent dust lanes are discernible. The morphology suggests a relatively evolved system, likely an elliptical galaxy that has undergone significant dynamical relaxation. There is no strong indication of recent major merger events, although a slight asymmetry suggests a possibility of minor past interactions. The galaxy's round shape implies a high degree of rotational symmetry.
