NGC_1975 is a bright emission nebula located in the constellation of Orion. It is part of a larger complex known as the Orion Nebula, which is one of the most studied regions of star formation in our galaxy. NGC 1975 is notable for its vivid colors and intricate structures, which are created by the interaction of stellar winds and radiation from young, hot stars with surrounding gas and dust. This nebula is approximately 1,600 light-years away from Earth and spans about 20 light-years across. It is often observed using telescopes, revealing details about the processes of star formation and the dynamics of interstellar matter. NGC 1975 contributes to our understanding of the life cycle of stars and the evolution of galaxies.