The galaxy presents a primarily smooth morphology with a hint of a disk-like structure. The overall shape appears mostly round, but with some deviation from perfect circularity. There is no evident sign of major disturbances or merging events. The galaxy exhibits a color gradient, with a reddish core region that fades to a more blue-green outer halo. This color gradient suggests the presence of older stellar populations concentrated in the center, with younger, bluer stars populating the outskirts.
