The galaxy appears to be undergoing a significant interaction, possibly a merger. It presents an irregular morphology with extended tidal features, indicative of gravitational disruption. Two distinct, bright nuclei are observed, one slightly more yellow, the other appearing whiter, suggesting different stellar populations or obscured active galactic nuclei. Diffuse emission surrounds both nuclei, with bluer hues present in some regions. The overall color gradient suggests ongoing star formation. The system appears relatively compact, and the bright nuclei indicate that it has a substantial stellar mass.
