NGC 1075 is a barred spiral galaxy located in the constellation Perseus. It is approximately 60 million light-years away from Earth and is part of a group of galaxies known as the NGC 1073 Group. This galaxy has a bright central bar structure and exhibits a well-defined spiral arm pattern. NGC 1075 is notable for its active star formation regions, which contribute to its luminosity and overall appearance. Observations of this galaxy help astronomers understand the dynamics and evolution of spiral galaxies in the universe.