This galaxy exhibits a clear spiral morphology. The spiral arms are loosely wound and appear to be asymmetrical. The color suggests active star formation is likely present, particularly within the spiral arms. There is a notable interaction, where two galaxies appear to be in the midst of a major merging event. One of the galaxies is much smaller, and the other one has a larger central bulge. There is no prominent bar structure visible, and the bulge size appears to be small relative to the overall disk. There are significant signs of major tidal disturbances and merging activity. 
