NGC 5867 is a planetary nebula located in the constellation Scorpius. It is approximately 3,000 light-years away from Earth and is known for its striking appearance, which includes a bright central star surrounded by a colorful shell of gas and dust. Discovered by John Herschel in 1834, NGC 5867 showcases the late stages of a star's life cycle. As the star expels its outer layers, the remaining core emits ultraviolet radiation, causing the surrounding gas to glow. This process contributes to the nebula's vibrant colors and intricate structure.