The galaxy appears to be undergoing a significant merger event. Two distinct galactic nuclei are visible, both exhibiting a yellowish-white hue, suggesting a population of older stars. Extensive tidal features or plumes are not clearly discernible, but there is a general elongation of the galaxy's structure. The overall color profile indicates a relatively low star formation rate. The shapes of the galaxies appear to be elliptical, not disk-like. 
