The distance to this system, as determined using parallax measurements, is approximately 162 light-years (50 parsecs).
[1] The system is a member of the Columba group of co-moving stars.
[12] This is an A-type main sequence star with a stellar classification of A1 V.[4] It is 317[9] million years old with a high rate of spin, showing a projected rotational velocity of 107 km/s.
It is radiating 27[6] times the Sun's luminosity from its photosphere at an effective temperature of 9,230 K.[4] The object displays an infrared excess, suggesting an orbiting debris disk with a temperature of 20 K at a mean radius of 932.40 AU from the host star.
[11] The system is an X-ray source with a luminosity of 16.57×1029 ergs s−1.