The galaxy presents a largely smooth, elliptical morphology. A concentrated central bulge is evident, exhibiting a yellowish-white hue, indicative of an older stellar population. This bulge is surrounded by a more diffuse halo of light, transitioning to a faint greenish-blue color towards the outer edges. The overall form appears relatively undisturbed, with no obvious signs of tidal features, spiral arms, or ongoing major mergers. The light distribution suggests a relatively high degree of rotational symmetry, although the galaxy appears slightly elongated along one axis. There may be some very minor disturbances happening. The galaxy's extended halo may be indicative of a supermassive blackhole in its center.
