The galaxy presents as a spiral, with a relatively faint, diffuse appearance. Two well-defined spiral arms are readily apparent, exhibiting a loose winding pattern. The arms appear somewhat patchy in color and brightness, suggestive of varying stellar populations and ongoing star formation. There is evidence of a central bulge, but it is not highly pronounced. Based on the visual disturbances and asymmetry present, the system appears to be undergoing a significant merger event. The overall morphology indicates an actively evolving system, likely influenced by gravitational interactions.
