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.
It is an isolated binary consisting of two main sequence stars that do not overflow their Roche lobes. The orbital plane is nearly aligned with Earth's line of sight, classifying it as a Beta Lyrae-type eclipsing variable star.