It is faintly visible to the naked eye with an apparent visual magnitude of 5.16.
[2] The annual parallax shift is 11.27 mas,[1] indicating a separation of around 289 light years from the Sun.
The star is around 600[7] million years old – 93%[3] of the way through its main sequence lifetime – and is spinning with a projected rotational velocity of 58 km/s.
[4] It is radiating 78[2] times the luminosity of the Sun from its photosphere at an effective temperature of about 9,000 K.[7] The star emits an infrared excess indicating the presence of a dusty debris disk.
The mean temperature of the dust is 85 K, indicating the semimajor axis of its orbit is 104 AU.