The combined apparent magnitude of 5.33[2] is bright enough to be seen with the naked eye.
Based upon an annual parallax shift of 14.09 mas,[1] the distance to this system is approximately 231 light-years (71 parsecs).
An excess of infrared emission suggests the presence of circumstellar dust in this system.
In the 24μm band, this debris disk has a mean temperature of 815 K, which puts it at a radius of 0.85 astronomical units (AU) from the primary star.
Excess emission appears in the 70μm band, which has a temperature of 103 K and a radius out to 42 AU.