The galaxy presents a face-on spiral morphology. The spiral arms are well-defined and exhibit a fairly tightly wound structure. Two distinct spiral arms are readily apparent. There appears to be a bar-like feature spanning across the central bulge region, bisecting the galaxy's core. The bulge constitutes a moderate fraction of the galaxy's overall size. No significant signs of a major merger are visibly distinct, however some possible minor disturbances may be present. Star formation may be taking place within the arm regions. The galaxy is not perfectly symmetrical, exhibiting some degree of morphological irregularity.
