A close binary star, with components of 4.8 magnitude (yellow) and 6.9 magnitude (red-orange), which have a mutual orbital period of 149 years. Since 1980, when they reached their maximum separation (7.2"), their separation has gradually decreased and currently reaches approximately 6". At the closest separation of 1.8" (last observed in 1918), the companion star is lost in small telescopes. The system is located 22 light-years away. In the field of view, at a distance of 99", another star HR 5553 (magnitude 6) usually appears, but it is not related to this system in any way.