[4] The distance to this star is approximately 487 light years based on parallax measurements, and it is drifting further away with a radial velocity of ~23 km/s.

[6] Simulations intended to reproduce the distribution of the circumstellar disk suggest an embedded planet with a mass of 6–9 MJ is orbiting the star at a distance of ~20 AU.

[9] Near infrared observations in 2018 show a spiral structure in the disk that is consistent with the presence of an orbiting planet.

[22] Observations with the Very Large Array during 2000 demonstrated the extent of the massive protoplanetary disk orbiting the star.

[25] Data from the Atacama Large Millimeter Array show a cavity in the inner disk that is depleted of gas and dust.