It is visible to the naked eye as a faint, white-hued point of light with an apparent visual magnitude of 4.82.

[2] The system lies approximately 209 light years away from the Sun based on parallax,[1] and is a member of the IC 2391 supercluster.

[8] It is moving closer to the Earth with a heliocentric radial velocity of −17 km/s.

[4] Radial velocity measurements from High Accuracy Radial Velocity Planet Searcher with an amplitude of 4 km/s indicate that it is a spectroscopic binary of unknown period.

[10] The star is an estimated 254[6] million years old with a relatively low projected rotational velocity of 52 km/s.