This galaxy appears to be composed of two distinct components. The first, and more prominent component, exhibits a relatively smooth morphology. The light from this area of the galaxy is concentrated towards the center and has a roughly circular shape, with what appears to be a bulge. The color of the light from the central region is more blue shifted than that of the secondary area. The second distinct area is more elongated and displays an overall redder shift. The elongated shape appears amorphous, possibly indicative of tidal disruptions or a more disk-like structure seen at an oblique angle. There seems to be no large scale merging events or extreme morphological disturbances, although one might identify subtle indications of minor gravitational interactions or disruptions. It seems the structure is more round than it is elliptical.
