NGC 6886 is a planetary nebula located in the constellation Cygnus. It is approximately 3,000 light-years away from Earth and is known for its distinct shape and bright central star. The nebula is formed from gas and dust ejected from a dying star, which creates a colorful and intricate structure. Discovered by William Herschel in 1788, NGC 6886 is part of a larger group of celestial objects known as planetary nebulae. These nebulae are often characterized by their round appearance and are typically the remnants of stars similar to our Sun that have reached the end of their life cycle.