The galaxy presents as a flattened, elliptical morphology. It exhibits a smooth light distribution, with a centrally concentrated bright core that appears to be slightly yellow. The outer regions fade gradually into the background, showing a slight disk-like structure. There's a subtle color gradient from the center outwards, suggesting a population shift from older stars in the core to potentially younger stars in the outer regions. No distinct spiral arms or prominent dust lanes are visible. There is a slight elongation, indicating it's not perfectly spherical, possibly an E3-E5 on the Hubble scale. There are no signs of tidal disturbances or ongoing major mergers.
