The galaxy presents as a merging system, exhibiting disturbed morphology. There are several distinct luminous regions, potentially representing the cores of the interacting galaxies or areas of enhanced star formation triggered by the interaction. The galaxy has an irregular shape, with a suggestion of tidal tails or bridges extending outwards, indicative of gravitational interaction. The color distribution is uneven, with concentrations of warmer yellow/orange hues contrasting with bluer peripheral regions, possibly reflecting variations in stellar populations or dust obscuration. Overall, the galaxy appears to be in a late stage of a merger event.
