The galaxy presents as a singular, extended object, suggesting a possible ongoing or recent interaction or merger. There appears to be a dual core structure or two distinct centers of luminosity, indicating two galactic nuclei in close proximity. The morphology is largely smooth with some indication of tidal features/disturbances, such as extended faint emissions, indicating there is an interaction and/or recent merger. There appears to be recent star formation within these cores and potentially throughout the galaxy. The object is slightly elongated, with a moderate axis ratio. Overall, the galaxy appears to be in an intermediate stage of merging or in post-merger stage with ongoing star formation and tidal disturbances.
