The galaxy appears as a faint, diffuse object with a bluish hue. It exhibits an irregular morphology, potentially indicative of ongoing interactions or recent mergers. There's a slight elongation suggesting it is a disk galaxy, and a brighter, somewhat amorphous central region. The low surface brightness suggests that this object may be relatively low mass. Evident disruptions point to a system undergoing significant gravitational disturbance, possibly a major merger event with another galaxy. The disturbed structures are likely areas of enhanced star formation.
