The galaxy appears to be in a state of merging, exhibiting a disturbed morphology. Two distinct, bright nuclei are visible, suggesting the recent interaction of two separate galactic structures. The overall color profile leans toward the redder end of the spectrum. There appears to be minimal dust extinction, implying a relatively clean line of sight through the merging system. Evidence for active star formation is subdued. Based on its estimated size and luminosity, this galaxy is considered to be massive. The merging process appears to be well underway. 
