The galaxy presents as a faint, relatively small spiral galaxy, seen at a significant angle. It appears to exhibit a disk-like structure, indicated by a slight elongation and hints of spiral arm morphology. Within the disk, there are localized regions of bluer light, possibly indicative of ongoing star formation. The overall color is generally redder, suggesting an older stellar population. Some disturbances and irregularities appear present throughout the disk, which may indicate ongoing or past merger activity.
