The galaxy exhibits a disturbed morphology, potentially indicating an ongoing or recent interaction. There is evidence of tidal features extending from the main galactic body. These features are diffuse and irregular, suggesting a complex interaction history. The galaxy's core region shows a relatively smooth appearance, however the surrounding disk presents evidence of asymmetry. There are multiple areas where the structure is irregular, which might reflect regions of star formation. Overall, the galaxy appears to be in a state of flux, with clear signatures of interaction or past merging events. The color distribution across the galaxy also suggests varying stellar populations or dust content.
