The galaxy presents as a system undergoing a significant interaction or merger event. The main body appears relatively smooth, with a primarily elliptical morphology. A second, smaller component is visibly interacting and appears to be in the process of merging. The system is relatively compact. There are significant tidal disturbances, with potential tidal tails or bridges of material emanating from the interacting galaxies. The system's color indicates that it is comprised of older stellar populations, with some star formation occuring. The roundness of the galaxy is high, with very little cigar shaping. Most volunteers indicate that this galaxy is in the midst of a merger.
