The galaxy presents a clearly defined disk structure and is not seen edge-on. Spiral arms are apparent and account for a considerable portion of the galaxy's luminosity. Two distinct, prominent arms can be discerned. The spiral arms exhibit a medium winding pattern. 

A bar feature seems present across the galaxy's center. The galaxy appears to be a spiral galaxy with a small to moderate bulge and the shape exhibits disturbances suggestive of a minor interaction or a merger. 
