The galaxy exhibits a distinct disk morphology, appearing relatively face-on. A spiral structure is evident, with at least two discernible arms. These spiral arms appear somewhat tightly wound. There is a central bulge region. The light distribution suggests that the bulge is not the dominant feature of the galaxy's morphology. There is a hint of a bar-like structure within the central region. There are no obvious signs of a major ongoing merger, though subtle disturbances might be present. The color distribution suggests active star formation within the spiral arms.
