The galaxy presents a discernible spiral structure. The spiral arms are prominent, exhibiting a relatively open winding pattern, not tightly coiled. Evidence suggests the presence of two major spiral arms. A bar-like structure is visible through the center of the galaxy, classified as being weak or of moderate intensity. A central bulge is identifiable, and although relatively small, it does contribute to the galaxy's overall structure. The galaxy is not edge-on. There is no major disturbance or major signs of merging, but some minor disturbances are present.
