The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge region that dominates the overall light profile. A diffuse, fainter halo surrounds the central region. There is a noticeable color gradient, with the central bulge appearing more red or yellow than the surrounding halo, indicating a population of older stars. No distinct spiral arms or prominent dust lanes are discernible. There is no evidence of major mergers or strong tidal disturbances. The overall structure suggests a galaxy that has undergone significant relaxation and is primarily composed of an older stellar population.
