Dusty galaxies are a type of galaxy that is classified based on the presence of large amounts of interstellar dust within their structure. This dust absorbs, scatters, and re-emits light, making dusty galaxies difficult to observe in optical wavelengths but easier to detect in infrared and submillimeter wavelengths. These galaxies are typically undergoing intense star formation processes, which produce copious amounts of dust as byproducts. Studying dusty galaxies can provide valuable insights into the formation and evolution of galaxies, the interplay between star formation and dust, and the role of dust in shaping galactic properties.