The galaxy presents as a relatively small, low-mass system. It exhibits a flattened, elongated shape, suggestive of a disk galaxy viewed at an oblique angle. The overall color appears bluish, indicating the presence of a young, hot stellar population and ongoing star formation. There are hints of structure within the disk, though these are not sharply defined; it's difficult to discern distinct spiral arms, but there are subtle variations in brightness across the disk that may indicate underlying spiral patterns. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or recent major mergers. There may be some low-level activity that would result in minor disturbances of the structure of the galaxy, but mostly it is a well formed disk galaxy. The central bulge is not very prominent, suggesting it's a late-type spiral or possibly an irregular galaxy.
