The system is fairly close, and is located about 76 light-years (23 parsecs) away, based on its parallax.
[1] Omega Draconis is a spectroscopic binary, which means the two stellar components are too close to be resolved but periodic Doppler shifts in their spectra indicate orbital motion.
In this case, light from both stars can be detected, and it is a double-lined spectroscopic binary.
[6] With 27 Draconis, it composed the Arabs' الأظفار الذئب al-ʼaẓfār al-dhiʼb, "the hyena's claws" in the asterism of the Mother Camels.
[9] Consequently, ω Draconis itself is known as 尚書一 (Shàng Shū yī, English: the First Star of Royal Secretary.).