The galaxy presents a generally smooth, elliptical morphology. There is a bright, concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. Surrounding the central bulge is a more diffuse halo, with a slightly bluer color index indicating the possibility of some younger stars. The galaxy appears relatively undisturbed, without obvious signs of ongoing or recent major mergers. The overall shape is close to round, deviating only slightly from perfect circularity. There may be some faint signs of a weak disk structure.
