The galaxy presents as a centrally concentrated, elliptical morphology. The light profile is smooth and diffuse, with a gradual decrease in intensity from the bright, unresolved nucleus outward. The core exhibits a yellowish hue, suggestive of an older stellar population. The outer regions appear fainter and redder, indicative of a more evolved stellar population or dust obscuration. No distinct spiral arm structures or dust lanes are discernible. The overall shape is moderately round. There is no evidence of tidal tails or other obvious signs of recent major merger activity. The galaxy appears relatively isolated and undisturbed.
