The galaxy presents a disk-like morphology with a noticeable spiral structure. The spiral arms appear well-defined, displaying a prominent two-armed pattern. The winding of these arms ranges from medium to tight. A central bar is present, showing a strong and distinct structure across the galaxy's nucleus. The bulge component appears relatively small. There is no evidence of significant mergers, only minor disturbances in the disk. The disk is not perfectly edge-on, but rather is tilted with a significant z-component visible. There are few regions of intense star formation apparent in the arms. The light is mostly in the blue spectrum, suggesting younger stellar populations.