NGC_2025 is a barred spiral galaxy located in the constellation Doradus. It is approximately 50 million light-years away from Earth and is part of the LMC (Large Magellanic Cloud), a satellite galaxy of the Milky Way. This galaxy is notable for its bright star-forming regions and distinctive spiral arms. NGC_2025 is often studied by astronomers to understand the processes of star formation and the dynamics of galaxies in the local group. Its proximity makes it an excellent target for observational research.