The galaxy presents as a smooth, elliptical-like structure. The central region displays a concentrated, yellowish-orange hue, potentially indicative of an older stellar population. This core transitions into a fainter, diffuse halo with a slight greenish tint, suggesting a more mixed stellar population or the presence of ionized gas. The overall shape is somewhat elongated, resembling a flattened spheroid, but there is a slight suggestion of a disk-like component. There is no evidence of strong spiral arms or active galactic nuclei activity visible within this image. The galaxy appears relatively isolated with no signs of major disturbances or ongoing mergers.
