The galaxy presents as a face-on spiral, exhibiting a disk structure with prominent spiral arms. The arms appear relatively well-defined and extend outward from a central bulge. The bulge appears moderate in size compared to the overall disk. There are two dominating spiral arms. The arms may be tightly wound. No strong bar structure is visible. The galaxy's disk demonstrates distinct color variations, indicating differing stellar populations within the structure. The galaxy shows no obvious signs of major disturbances that may be attributed to a merger.
