The galaxy presents a generally smooth morphology, suggesting a relatively evolved system. It exhibits a slightly elongated shape, appearing more oblate than perfectly spherical. The light distribution is concentrated towards the center, indicative of a prominent galactic bulge. Faint, diffuse features that might be indicative of spiral arm structures are present, although poorly defined. There are no prominent signs of major mergers or tidal disturbances. Overall, this galaxy seems to be a relatively undisturbed and passively evolving system.
