B型主系列星
Howe and Clarke (2009) catalog this as a double-lined spectroscopic binary star system with a wide projected separation of . As of 2018, they had an angular separation of along a position angle of 30°. The brighter member, component A, is a B-type main-sequence star with a stellar classification of B1V. The secondary, component B, is of class B3V. Both stars are spinning rapidly.