The galaxy presents a largely smooth morphology, with a dominant central bulge. There is a subtle disk-like structure surrounding the bulge, though its features are indistinct. The overall shape is elliptical, but noticeably departs from perfect circularity, trending toward a more elongated form.  There are no obvious signs of spiral arms or bar structures. Color gradients are visible, with the central bulge appearing more yellow/orange, indicative of an older stellar population. The outer regions of the galaxy are slightly bluer. There's no evidence of on-going major merging activity, although some faint asymmetry suggests the possibility of a minor interaction in the past. The galaxy's light distribution appears centrally concentrated, but tapers off gradually toward the edges.