It is faintly visible to the naked eye with an apparent visual magnitude of +5.46.

[2] Based upon an annual parallax shift of 8.31 mas as seen from the Earth,[1] the star is located roughly 390 light-years from the Sun.

This is a single-lined spectroscopic binary system with an orbital period of 3.8 years and an eccentricity of 0.35.

The primary, component A, is a white-hued A-type giant star with a stellar classification of A0 III.

[3] It is a magnetic Ap star with a field strength of 846×10−4 T, showing abundance peculiarities in strontium, chromium and mercury.