The galaxy presents a largely smooth morphology. The light distribution is highly concentrated toward the center, with a gradual decrease in luminosity outwards. The core region exhibits a bright, nearly uniform, intensity. The overall shape appears nearly circular, showing a high degree of rotational symmetry. There are no discernible spiral arms or a prominent disk structure. There are no obvious signs of tidal disturbances or ongoing merger activity. Faint color gradients are present. The central region exhibits a slightly yellower color than the outer regions, possibly indicative of an older stellar population. Overall, the galaxy appears to be a well-formed elliptical galaxy.
