The galaxy presents as a face-on spiral structure. Two well-defined spiral arms are visible, extending outwards from a central bulge. These arms appear relatively loosely wound. The color distribution across the galaxy suggests ongoing star formation, with bluer hues concentrated in the spiral arms, indicative of the presence of young, hot stars. A weak bar structure may exist across the center. There are visible signs of a merger or tidal disturbance, as the arms and overall structure look to be disrupted, and there is an apparent dwarf galaxy being merged in the process. The bulge appears smaller in relation to the disk. 
