The galaxy appears to be a spiral galaxy viewed at a slight angle. There is evidence of distinct spiral arms, relatively tightly wound, emanating from the central bulge. The galaxy's color suggests it is a star forming galaxy. The central bulge exhibits a moderate size in relation to the overall disc. There is a hint of a bar-like structure bisecting the central region. The galaxy's disk presents as slightly uneven. No major signs of ongoing merging are observed, but there seems to be minor disturbances in the symmetry of the spiral arms.
