The galaxy appears to be undergoing a significant merger event. Two distinct luminous components are visible, seemingly gravitationally interacting and distorting each other's shapes. The larger, more diffuse component exhibits a yellowish hue, potentially indicating an older stellar population or a higher concentration of dust. A second, smaller, and somewhat bluer component is located nearby, suggesting ongoing or recent star formation. The overall morphology is highly irregular, lacking a well-defined spiral or elliptical structure, and the primary bodies have been observed to be strongly interacting, making tidal distortions highly likely.
