The galaxy presents as a complex interacting system. A prominent spiral structure is evident, displaying loosely wound arms. The arm count appears to be dominated by a two-arm morphology. 

A strong interaction is indicated, with a portion of the galaxy significantly disturbed. The morphology suggests a major disturbance, possibly a merger in progress. There is a feature with high surface brightness which could be evidence of active star formation or potentially tidal debris. It is difficult to discern the presence of a bar. The bulge appears to be of small to moderate size. 
