The galaxy presents a spiral morphology with a defined disk structure. Evident spiral arms extend from a central bulge. The winding of the arms is relatively loose. There is a presence of two dominant spiral arms. The galaxy appears to be undergoing a significant interaction or disturbance, as indicated by the asymmetry and some features in the disk. There seems to be a small to moderate bulge at the center, and perhaps a weak bar. The color distribution suggests ongoing star formation, concentrated within the spiral arms.
