It is a detached binary with two main sequence components that do not fill their Roche lobes. The orbital plane is oriented near the line of sight from the Earth, making this a Beta Lyrae–type eclipsing binary variable star.
This binary consists of two main sequence components that do not exceed their Roche lobes; the orbital plane is nearly parallel to our line of sight from Earth. Consequently, this system behaves like a Beta Lyrae-type eclipsing binary variable star.