The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, surrounded by a more diffuse halo. Color gradients are apparent, with the central region showing a yellowish-white hue, indicative of an older stellar population, potentially dominated by evolved red giant stars. The outer regions appear slightly bluer, suggesting the presence of a younger stellar population, though not prominently so. There is no clear evidence of distinct spiral arms or a disk-like structure. Overall, the galaxy appears to be a relatively undisturbed system, with no major signs of ongoing mergers or tidal interactions.
