This galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated core. The light profile appears to fade gradually from the center outwards, with no distinct spiral arm structures or prominent dust lanes visible. There is a slight color gradient, shifting from a yellower hue in the core to a bluer tint in the outer regions, possibly indicating a difference in stellar populations. The galaxy appears relatively isolated and undisturbed, with no obvious signs of tidal interactions or major mergers, although some minor disturbances cannot be ruled out. The overall appearance suggests a relatively mature system, potentially undergoing some continued star formation.
