The galaxy presents as a centrally concentrated, smooth object. It exhibits a nearly circular morphology, with no immediately apparent spiral arm structures or significant asymmetries. The central region appears considerably brighter than the surrounding areas, suggesting a dense stellar population or possibly an active galactic nucleus. Coloration appears relatively uniform throughout the galaxy, tending towards bluer hues. There is no obvious indication of major ongoing merger activity, although faint hints of minor disturbances can be observed in the outer regions. Based on the apparent smoothness and roundness, this galaxy is likely an elliptical galaxy.