 It is about 2.2 times the size of the Sun and is radiating 37 times the Sun's luminosity from its photosphere at an effective temperature of 9,141 K.

The secondary, component B, is magnitude 8.68 star with an angular separation of from the primary, as of 2008.X-ray emission has been detected from this system.As A-type stars are not expected to be X-ray sources, this emission is most likely coming from the companion.