NGC 261, located in the Small Magellanic Cloud, is an emission nebula that has caught the attention of astronomers using the Hubble Space Telescope. This diffuse region, about 200,000 light-years away in the constellation of Tucana, is a focal point for studying star formation in molecular clouds. The nebula's pinkish-red glow results from hot stars interacting with surrounding hydrogen gas, offering valuable insights into the process. By examining the carbon monoxide content using Hubble's Advanced Camera for Surveys and Wide Field Camera 3, scientists aim to unravel the mechanisms behind star birth in not only NGC 261 but also in similar regions within our galactic neighborhood. This research showcases the intricate relationships between molecular clouds, star formation, and the evolution of galaxies, ultimately contributing to a deeper understanding of the cosmos.