The galaxy exhibits a disturbed morphology, suggesting an ongoing or recent interaction. There's evidence of tidal features or asymmetries in the galactic structure. The light appears to be relatively blue overall, possibly indicating a younger stellar population and ongoing star formation, particularly in the central regions. The galaxy may be undergoing a merger, as indicated by the distorted shape and potential tidal tails or bridges. It presents as a fuzzy object, with ill-defined spiral arms or a disrupted disk. Patches of enhanced brightness are observable, potentially corresponding to star-forming regions or knots of accumulated stellar material. The size of the galaxy appears relatively compact.
