The galaxy appears to be undergoing a significant interaction or merger event. There are two distinct luminous cores, suggesting the presence of at least two galactic nuclei. One core is brighter and more diffuse than the other. The overall shape is highly irregular and distorted, with evidence of tidal features or disrupted spiral arms. The color of the galaxy is predominantly yellowish, indicating an older stellar population and a lower rate of ongoing star formation. There are suggestions of bluer regions, possibly areas of recent star formation triggered by the interaction. Overall, it is difficult to classify this galaxy under traditional morphological types due to the clear signs of disruption.
