The galaxy presents as a centrally concentrated object with a smooth overall morphology. Its shape appears somewhat elliptical, neither perfectly circular nor significantly elongated. The core region exhibits a yellowish hue, suggestive of an older stellar population. The light appears to fade gradually from the center outwards, forming a diffuse halo. There may be faint hints of a disk structure, but it is not sharply defined. There's no obvious evidence of ongoing major mergers, though minor disturbances may be present. Overall, the galaxy appears relatively undisturbed and evolved.
