The galaxy presents an overall elliptical morphology, although there is some indication of a possible disk structure. The light distribution is fairly smooth, with a centrally concentrated bulge region that exhibits a slightly brighter and more defined core. While the galaxy appears largely undisturbed, there are hints of subtle irregularities in the outer regions, possibly indicating minor gravitational interactions or past merger events. Color gradients appear consistent with an older stellar population, though a hint of bluer color in the central area suggest ongoing star formation. It is primarily smooth, with some indication of a slight disk structure. The galaxy exhibits an approximately round shape.
