The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution indicates a likely evolved stellar population, exhibiting a yellowish-red hue across its body, indicating older stars. There is a hint of a disk, but the light appears to be dominated by the bulge. The galaxy appears to be relatively isolated, with no obvious signs of recent major mergers or significant tidal disturbances in this image. It presents as a fairly regular, non-interacting system at a significant distance, with its shape appearing to be more in between round and elliptical, with a slight lean toward being elliptical.
