The galaxy presents as an interacting system, exhibiting characteristics indicative of an ongoing or recent merger event. The morphology appears disturbed with an irregular shape. There is an apparent dual core structure, with a prominent, bright central region appearing yellowish in color, likely indicating an older stellar population and a secondary core exhibiting a bluer hue, suggesting ongoing star formation. A faint tidal tail extends outward from the main body. The overall color suggests a mix of stellar populations and possibly dust obscuration within the system.
