This system was found to be a close double-lined spectroscopic binary in 1977, consisting of two B-type main-sequence stars. It has a near circular orbit with a period of 15.727 days and a semimajor axis of . They appear to be spin-orbit synchronized.
In 1977, this system was identified as a close double-lined spectroscopic binary consisting of two B-type main-sequence stars. It orbits with an almost circular path having a period of 15.727 days and a semimajor axis of . The stars appear to be spin-orbit synchronized.