The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which transitions smoothly into a more diffuse outer region. The galaxy's color is primarily yellowish-red, which might indicate an older stellar population with lower rates of current star formation. There is a slight elongation or asymmetry. No prominent spiral arms or distinct dust lanes are discernible at this resolution. Any features indicating ongoing mergers or tidal disturbances appear minimal; this galaxy seems relatively undisturbed.
