It was the first fully resolved triple T-type brown dwarf system that was discovered.

Follow-up observations with Keck/OSIRIS resulted in resolved spectrum of the A and the BC components.

Components BC have a relative small separation of around 2.5 AU and should have an orbital period of around 12 or 21 years.

The researchers find that for an age of 3 billion years the system would have a gravitational binding energy of about 20 × 1041 erg.

For an age of 300 million years, the gravitational binding energy is about 1.6 × 1041 erg, which would make it a rare weakly bound triple.