The galaxy presents a morphology suggesting an ongoing or recent merger event. It exhibits a centrally concentrated luminosity profile, with a smooth texture and an overall elliptical shape. There appear to be two distinct, bright cores within the galaxy, indicative of two galactic nuclei in close proximity. The color of the galaxy is primarily yellow, which suggest an older stellar population with reduced star formation rate. There is a low probability of disk components and a moderate probability of it exhibiting merging characteristics. The object's morphology aligns with an evolved system where major interaction is occurring.
