The galaxy presents a disk-like morphology, exhibiting discernible spiral arm structure. These arms appear somewhat tightly wound. A central bulge is observed, although its size appears to be moderate. The overall light distribution suggests a relatively normal spiral galaxy, with no obvious signs of a major ongoing merger, although there might be some evidence of minor disturbance. The disk's orientation is nearly face-on. The galaxy's color suggests a mixture of stellar populations, implying ongoing star formation. There is no clear bar-like structure visible. The galaxy is not perfectly smooth.