The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, exhibiting a high degree of circular symmetry. There's a noticeable color gradient, shifting from a yellowish-white hue at the core to a bluer tint in the outer regions, indicating a possible distribution of younger stars in the outskirts relative to the core. There is no clear evidence of spiral arm structure, bars, or other defined features such as tidal tails or dust lanes suggesting a merger event. Some minor disturbances cannot be ruled out, but the object seems to be quite round and mostly undisturbed.
