The galaxy appears to be an interacting pair, exhibiting a disturbed morphology. Both galaxies possess elliptical shapes, and seem to be in the midst of a major merging event. Some tidal tails or bridges, faint and diffuse, may be present and there seems to be a higher degree of concentration toward their centers. The overall color profile suggests a relatively mature stellar population with a moderate amount of dust extinction, with a higher concentration of redder stars. There is an apparent axis of symmetry along the longer axis of the larger galaxy.
