The galaxy appears to be undergoing a major merger. Three distinct luminous components are visible, suggesting either a merger of three galaxies or a binary merger with a tidal dwarf galaxy. The components exhibit a smooth morphology, with no clear spiral arm structure visible in any of the merging galaxies, although the presence of green suggests that there is ongoing star formation. The color is reddish, which is characteristic of older stellar populations, but the hint of green implies regions of active star formation. The overall shape is complex, indicating a disturbed system likely far from dynamical equilibrium. This galaxy shows strong signs of interaction, possibly leading to a single, more massive elliptical galaxy in the future.
