NGC 6744A is a spiral galaxy located approximately 30 million light-years away in the constellation Pavo. It is part of the NGC 6744 galaxy group and is often considered a satellite of the larger NGC 6744 galaxy. This galaxy exhibits a well-defined spiral structure, featuring bright regions of star formation and a central bulge. NGC 6744A is notable for its resemblance to the Milky Way, showcasing similar characteristics such as spiral arms and a disk-like shape. Its study helps astronomers understand the formation and evolution of spiral galaxies.