The galaxy presents as a somewhat elongated structure with a distinct morphology suggestive of a late-stage merger or strong tidal interaction. One end of the galaxy is brighter and bluer than the rest of the galaxy, and it contains some internal structure. The opposite end of the galaxy is more diffused, more centrally condensed, and has a redder color. A relatively faint bridge of material connects the two brighter ends. The overall shape of the system is irregular, possibly influenced by gravitational interactions. The distribution of light across the galaxy is not uniform.
