The galaxy presents as a roughly elliptical structure, characterized by a smooth overall morphology. A bright, concentrated central bulge is evident, exhibiting a yellowish hue suggestive of an older stellar population. Fainter, bluer regions extend outwards from the core, displaying a disk-like component. The disk shows only subtle hints of spiral arms, and instead it is mostly diffuse and patchy in nature. There are some signs of minor disturbance, indicated by slight distortions in the shape of the outer disk.
