IC 1271 is a planetary nebula located in the constellation of Aquarius. It is approximately 2,500 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. The central star of IC 1271 is a white dwarf, which is the remnant of the original star that has shed its outer layers. As the white dwarf continues to heat up, it illuminates the surrounding gas, causing it to glow. This process contributes to the nebula's beauty and complexity, making it a subject of interest for astronomers.