The galaxy presents a disk-like structure viewed at an oblique angle. Prominent spiral arms are visible, exhibiting a loosely wound morphology. The arms display a clumpy structure, suggesting active star formation regions. These regions appear bluer in color, indicative of the presence of hot, young stars.

A moderate bulge is discernible at the galaxy's center, although it does not appear to be the dominant feature. The overall color of the galaxy appears relatively blue. The structure appears mostly undisturbed, with no clear signs of major merging events, though the presence of minor disturbances cannot be ruled out. The galaxy does not appear to have a strong bar structure.
