The galaxy appears to be a spiral galaxy, observed at an angle between face-on and inclined. Its spiral arms exhibit a grand design structure, appearing flocculent with areas of active star formation, evidenced by the clumpy distribution of light. The color profile suggests ongoing star formation, the arms being bluer than the central bulge. A central bulge is observed and the distribution of light implies it is moderate in size compared to the disk component. There is no obvious bar structure visually apparent in the image. The morphology is relatively undisturbed, indicating a lack of recent major merger events. The arm winding is of mixed type, showing both tightly wound and loosely wound regions throughout its structure. Two dominant arms are easily visible, but there are also more, branching arm segments.