This galaxy appears to be a merging system, potentially in its later stages of interaction. The overall morphology is complex and irregular. Two distinct, luminous cores are visible, with diffuse emission extending between them. One core exhibits a yellow-white hue, suggesting an older stellar population, while the other shows a more reddish tint, potentially indicative of ongoing star formation or dust obscuration. There is some evidence of tidal features, with faint extensions. The galaxy does not display a clear disk or spiral structure, appearing primarily elliptical or spheroidal in shape. The system shows a generally smooth appearance, with some perturbations that can be caused by galaxy merging. The presence of both older and potentially younger stellar populations indicates a complex and dynamic star formation history within the merging galaxies. The system is relatively compact.
