NGC 6779 is a globular cluster located in the constellation of Aquarius. It is approximately 30,000 light-years away from Earth and is part of the Milky Way galaxy. This cluster is notable for its dense concentration of stars, which are primarily older, metal-poor stars. Discovered by William Herschel in 1784, NGC 6779 is classified as a type II globular cluster. It has an apparent magnitude of around 10.5, making it visible through small telescopes. The cluster's age is estimated to be around 12 billion years, providing valuable insights into the early formation of the galaxy.