NGC 1975 is a bright emission nebula located in the constellation Orion. It is part of a larger complex known as the Orion Molecular Cloud, which contains several other notable nebulae, including NGC 1973 and NGC 1977. This nebula is approximately 1,500 light-years away from Earth and is known for its striking colors and intricate structure. The nebula is illuminated by the intense radiation from nearby young stars, which causes the surrounding gas and dust to glow. NGC 1975 is often studied by astronomers to understand star formation processes and the dynamics of interstellar matter in our galaxy, the Milky Way.