The galaxy appears as a concentrated, elliptical-like structure. It exhibits a smooth, centrally-concentrated morphology, with a distinct core region, possibly with a disk-like appearance. There is a color gradient visible, with the central region exhibiting a yellowish hue, which could be indicative of an older stellar population or dust obscuration. The outer regions of the galaxy seem to have a bluer tint, possibly indicating the presence of younger stars and ongoing star formation, although at a low rate. There are some suggestions of minor disturbances in the morphology of the galaxy but it is subtle, with no major merging or tidal features readily apparent.
