The galaxy exhibits characteristics suggestive of an ongoing or recent merger event. The morphology is complex, with evidence of disrupted structure. Two distinct, bright nuclei are observed, one with a bluer color and the other more yellow, implying differing stellar populations. The galaxy appears to be undergoing gravitational interactions, as indicated by the disturbed morphology and potential tidal features. There is some evidence of diffuse light surrounding the galaxy, potentially representing a halo of stars ejected during the interaction.
