The galaxy exhibits a prominent spiral structure, with arms that appear loosely wound. The disk component dominates the overall morphology. The central bulge is relatively small in comparison to the disk. The light distribution suggests the presence of two dominant spiral arms. There is no obvious indication of significant interaction or merging events, although there are some disturbances in the disk. A weak bar structure appears to be present. Based on the color gradients, this galaxy hosts ongoing star formation, particularly in the spiral arms. The galaxy shows some bluer regions, suggesting that is where it might be forming the most stars. The color indices are consistent with an intermediate-redshift galaxy.