This galaxy appears to be undergoing a significant merging event. The system exhibits a disturbed morphology, with two distinct, luminous cores. These cores are likely the remnants of the original galactic nuclei. The overall light distribution is irregular and asymmetric. The colour profile shows a concentration of older stellar populations in the central regions, indicated by the yellow-red hue. Hints of bluer light are also present, suggesting the existence of some star formation activity. Evidence of tidal tails or extended debris is not very prominent, however, based on the morphology, a substantial fraction of the light is related to on-going merging and interaction. The object's overall appearance suggests a relatively evolved system.
