The galaxy presents as a fairly elliptical, smooth object. A concentrated central bulge of older stars is present. Fainter, diffuse light extends beyond this central region, displaying a slightly flattened, disk-like structure. This outer region shows hints of bluer colors, which could indicate regions of recent star formation. Overall, the galaxy lacks any obvious spiral arm structure or major disturbances, suggesting it is a relatively undisturbed system and may be a lenticular or early-type spiral. 
