It is visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 5.72.
[2] This object is located approximately 335 light years distant from the Sun, based on parallax, and is drifting further away with a radial velocity of +18 km/s.
This object is an A-type main-sequence star with a stellar classification of A0V.
[3] It is 94[5] million years old with a high rotation rate, showing a projected rotational velocity of 149.
[5] The star has 2.46[5] times the mass of the Sun and is radiating 49[6] times the Sun's luminosity from its photosphere at an effective temperature of 10,325 K.[7] It is the southern pole star of Venus.