The galaxy presents a distinct spiral structure, exhibiting prominent arms that wind around the central bulge region. These spiral arms appear somewhat fragmented and exhibit varying degrees of tightness. The arms are predominantly blue, suggesting ongoing star formation. The central bulge is moderately sized and shows a yellowish hue, possibly indicative of an older stellar population. The disk of the galaxy is clearly visible and not edge-on. There is evidence of disturbance within the galaxy, possibly due to a minor interaction or merger, as indicated by some asymmetry and irregular features within the spiral arms. There may be a weak bar feature present in the center of the galaxy. There is a single, strong spiral arm present.