The galaxy presents a somewhat amorphous structure, lacking well-defined spiral arms or a distinct central bulge. The overall color gradient suggests a dominance of older stellar populations, although some regions display bluer hues, potentially indicative of ongoing or recent star formation. The galaxy appears relatively isolated, showing no obvious signs of interaction with other galaxies. The morphology is primarily smooth, but there are some features suggestive of a disk. There is a hint of some minor disturbances.
