The galaxy exhibits a morphology characteristic of a spiral galaxy, displaying distinct spiral arm structures. The arms appear somewhat loosely wound and flocculent, with bright knots of star formation evident along their lengths. There appears to be a weak bar structure in the central region of the galaxy. The bulge component seems relatively small or possibly non-existent, as the galaxy's light distribution is dominated by the disk.

There is evidence of potential interaction or merging activity. The overall form of the galaxy is perturbed, exhibiting some degree of asymmetry. The galaxy displays a blue color, which indicates a presence of active star formation within the disk. The estimated size of the galaxy is consistent with being a normal-sized spiral galaxy.
