The galaxy presents a diffuse, somewhat irregular morphology. It appears to be a spiral galaxy with a low inclination relative to our line of sight. The central bulge is not particularly prominent, suggesting a smaller bulge-to-disk ratio. Spiral arms are visible but are somewhat flocculent and not tightly wound. Patches of bluer light, indicating regions of active star formation, are distributed throughout the disk. The overall color of the galaxy leans toward the blue end of the spectrum, consistent with ongoing star formation. There is some indication of tidal disturbances or interactions, as the galaxy's structure looks slightly distorted.
