The galaxy presents an overall elliptical morphology, appearing as a smooth, centrally concentrated object. The core region exhibits a yellowish hue, which could indicate an older stellar population. A fainter, bluer, diffuse halo surrounds the core, hinting at the presence of a younger stellar population possibly undergoing some star formation. The galaxy displays an intermediate ellipticity, leaning more towards a rounded shape than a highly elongated form. There are no obvious signs of major mergers or strong tidal disturbances in the immediate vicinity, though there might be some minor disturbances. Overall, the galaxy appears relatively isolated and unperturbed.
