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.
This system was identified as a close double-lined spectroscopic binary in 1977, comprising two B-type main-sequence stars. It has an almost circular orbit with a period of 15.727 days and a semimajor axis of . They seem to be spin-orbit synchronized.