IC_1295 is a planetary nebula located in the constellation Centaurus. It is known for its striking appearance and is part of a larger group of nebulae that are formed from the remnants of dying stars. The nebula emits light due to the ionization of gas surrounding the central star, creating a colorful display. Discovered in the late 19th century, IC_1295 is approximately 2,000 light-years away from Earth. Its central star is a hot, luminous object that contributes to the nebula's brightness. Observations of IC_1295 help astronomers understand the life cycle of stars and the processes involved in nebula formation.