IC 449 is a planetary nebula located in the constellation of Aquarius. It is part of a group of celestial objects known for their distinct shapes and colors, formed from the outer layers of a dying star. The nebula is approximately 2,000 light-years away from Earth and is notable for its intricate structure. The central star of IC 449 is a white dwarf, which is the remnant of the original star that created the nebula. As the star expels its outer layers, it emits ultraviolet radiation that ionizes the surrounding gas, causing it to glow. This process contributes to the nebula's vibrant appearance.