A binary star (with stars of 4.4 magnitude and 8.6 magnitude, angular separation of 35.9'') can be resolved with a small telescope with a 6 cm objective diameter. The primary component has an absolute magnitude of -1.1, is 170 times more luminous than the Sun, and is located at a distance of 600 light-years. In a telescope with a 200mm objective diameter, it appears as a bright white star with a faint bluish companion. A faint star of magnitude 13 is also projected in the vicinity.