This galaxy exhibits characteristics suggestive of a spiral morphology. There is evidence of a disk structure, though it seems partially obscured or disturbed. Distinct spiral arm features are visible, exhibiting a clumpy structure, indicative of regions of active star formation within the arms.

There is some visual evidence of possible tidal disturbances or interactions with another galaxy. The galaxy's morphology shows an irregular pattern. The galaxy appears to show minor signs of a possible merging event.
