NGC 1058 is a spiral galaxy located in the constellation Cassiopeia. It is approximately 40 million light-years away from Earth and is part of the Messier 101 group of galaxies. NGC 1058 has a diameter of about 50,000 light-years and is classified as a type Sc spiral galaxy. This galaxy is notable for its bright core and well-defined spiral arms, which contain regions of active star formation. NGC 1058 is also home to several supernova remnants, making it an interesting object for astronomers studying stellar evolution and the life cycle of galaxies.