The galaxy presents a largely smooth, elliptical morphology. There is little discernible disk structure, no apparent spiral arms, and the light profile suggests a centrally concentrated bulge component. The galaxy exhibits a color gradient, appearing bluer towards the core. The overall light distribution appears generally symmetrical, with no prominent tidal features or strong indications of ongoing major merger activity. There is a suggestion of minor disturbance within the galaxy, but is mostly a homogenous structure.
