The galaxy appears to be undergoing a merger or significant interaction. Two distinct luminous regions are visible, possibly representing the cores of the merging galaxies. The system exhibits an overall irregular shape, deviating significantly from a classical spiral or elliptical morphology. There may be potential tidal tails or bridges of material extending from the main body of the galaxy, though this is not definitive.

The colour gradients indicate the presence of distinct stellar populations and/or dust lanes, with the central regions exhibiting bluer hues suggestive of ongoing star formation. Redder regions are also visible, possibly indicating older stellar populations or regions obscured by dust. The overall structure is complex and disturbed, suggesting that the system is in a highly dynamic state.
