The galaxy exhibits a spiral structure. Its disk is observed at a relatively face-on orientation, displaying prominent spiral arms. The arms appear somewhat fragmented and flocculent, suggesting ongoing star formation. The galaxy possesses a noticeable bulge, approximately moderate in size, although it does not dominate the overall structure. A bar-like structure seems to be present across the galaxy, though it is not distinctly strong, and has a weaker presence in the center of the bulge. There is no obvious signs of ongoing major merging events. The HI data shows a relatively wide spectral width.