The galaxy presents as a single, relatively smooth object. Its overall morphology appears elliptical. The central region exhibits a high degree of concentration and a yellowish hue, suggesting an older stellar population. The outer regions fade gradually, exhibiting a bluer tint. There is no evidence of spiral arms or a prominent disk. The galaxy's shape is somewhere between round and elliptical. No signs of tidal tails, major mergers, or other significant disturbances are apparent, although a slight asymmetry cannot be ruled out.