The galaxy exhibits a morphology indicative of an ongoing merger event. Two distinct galactic nuclei are discernible, connected by a faint bridge of material. One nucleus appears more compact and exhibits a smoother light distribution, with a predominantly redder hue. The other nucleus appears more diffuse with an irregular shape. There are indications of tidal distortions, although no clear tidal tails are observed. Overall, the system exhibits a complex structure resulting from the gravitational interaction of two galaxies in the process of merging. The colors suggest the possibility of moderate star formation within one or both of the interacting galaxies.
