The galaxy presents a distinct spiral morphology. Two prominent spiral arms are visible, tracing outwards from a central bulge region. The arms exhibit a moderate winding, neither tightly wound nor significantly extended and loose. The bulge appears relatively small compared to the overall galactic disk. The disk exhibits a mottled texture, suggestive of ongoing star formation regions. The galaxy is not obviously edge-on; instead, it's observed at a moderate angle, allowing good visibility of the spiral structure. There's no clear indication of a bar structure bisecting the central bulge, nor any strong signs of a recent major merger event. Slight color variation is observed, with bluer hues visible along the arms.