The galaxy presents a somewhat elliptical morphology, appearing neither perfectly spherical nor highly elongated. The light distribution indicates a relatively smooth profile, lacking prominent spiral arms or a distinct bar structure. There is a central concentration of light, suggesting the presence of a galactic nucleus or bulge. The overall color appears bluish, which could indicate the presence of younger, hotter stars and possibly ongoing star formation, albeit at a relatively low rate. There is no obvious indication of any major mergers or significant tidal disturbances. Minor irregularities may be present in the outer regions, but overall the galaxy appears to be relatively undisturbed.
