IC 1295 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. Planetary nebulae like IC 1295 are formed when a star similar to our Sun exhausts its nuclear fuel and sheds its outer layers, creating a glowing shell of gas. The central star of IC 1295 is a hot, luminous object that emits ultraviolet radiation, causing the surrounding gas to ionize and emit light. This process gives the nebula its colorful appearance, which can be observed through telescopes. IC 1295 is an interesting object for astronomers studying the life cycle of stars and the evolution of nebulae.