The galaxy presents as a spiral type, exhibiting a relatively high degree of disk structure. The arms are clearly defined and appear to wind relatively tightly around the central bulge. A moderate central bulge is observed, with a luminosity that decreases gradually outward into the disk. The galaxy shows a distinct blue tint within the spiral arms. Dust lanes are evident, creating some level of obscuration within the spiral arms. There appears to be some mild distortion to the overall morphology. The galaxy exhibits a slight ellipticity.
