This galaxy appears to be undergoing a significant interaction or merger. The morphology is disturbed, exhibiting an irregular shape and a complex internal structure. There is evidence of tidal features or disrupted arms, indicating gravitational interaction with another galaxy or multiple galaxies. One distinct, relatively compact, bright blue region may be a site of enhanced star formation, potentially triggered by the interaction. The overall color of the galaxy appears to be relatively blue, suggesting the presence of a younger stellar population. There are areas of apparent dust extinction, but no well-defined spiral arms or a prominent bulge. The presence of what appear to be minor disturbances suggest a possibility of tidal interactions with other galaxies. The light output is concentrated to the central region of the system. 
