The observed galaxy appears to be undergoing a significant merger. Two distinct galactic nuclei are visible, both exhibiting a yellowish-orange hue, suggesting an older stellar population. Tidal features are subtly visible in the surrounding space, indicating gravitational interaction and disruption of the original galactic structures. The system displays an overall amorphous shape, lacking a clear spiral or elliptical structure, further supporting the merger hypothesis. There is some blue within the tidal debris, suggesting some star formation is present. This suggests a galaxy in a relatively advanced stage of merging, potentially evolving toward a more homogenous elliptical morphology.
