The galaxy exhibits a primarily smooth morphology, with a high degree of central concentration. The light distribution suggests an elliptical or lenticular classification. The core region is bright and yellowish, indicating an older stellar population. Moving outwards from the core, the galaxy transitions to a greenish hue, possibly indicative of some ongoing, though subdued, star formation. There is no obvious presence of spiral arms or a distinct disk structure. The galaxy appears relatively undisturbed, showing no major signs of tidal interactions or ongoing mergers. It appears nearly round. The object's red shift indicates that it is a distant galaxy.