The galaxy presents a largely smooth morphology with a concentrated central bulge that appears yellowish. There is a fainter, bluer halo surrounding the central region. The galaxy appears relatively undisturbed, without any obvious signs of ongoing mergers or major tidal interactions. The overall shape is close to circular. There is a hint of a disk or a flattened structure, but it is subtle. The color gradient suggests that the central region consists of an older stellar population. The outer regions, which are bluer, could contain younger stars that formed from an ongoing star formation process.
