The galaxy appears to be undergoing a significant interaction or merger. Two distinct luminous cores are visible. The larger, primary core exhibits a yellowish-orange hue, suggesting an older stellar population, potentially an elliptical galaxy morphology. A secondary, smaller core displays a distinctly blue color, indicative of ongoing star formation with a younger stellar population. This likely is from an infalling galaxy. The overall structure is disturbed, lacking a clear spiral or elliptical shape, supporting the ongoing interaction hypothesis. There is faint light surrounding each of the two cores. Overall, the system presents a dynamic scenario of galactic evolution.
