The galaxy exhibits a clear spiral structure, with two prominent arms emanating from the central region. These arms appear loosely wound and are traceable for a considerable distance. The disk is viewed at an angle that is slightly offset from face-on, and appears disturbed. There is evidence of ongoing star formation along the spiral arms as indicated by the clumpy structures of relatively blue hue. The central bulge presents a moderate size relative to the disk, exhibiting a yellower hue. There is the possibility of a bar-like structure extending through the center of the bulge, it's morphology however is hard to properly visualize.

The morphology suggests possible ongoing or recent interaction with another galaxy. Several disturbed components are visible, including what appears to be a tidal tail and several merging companions.
