NGC 2407 is a spiral galaxy located in the constellation Camelopardalis. It is approximately 10 million light-years away from Earth and is part of the M81 Group, which includes several other galaxies. Discovered by William Herschel in 1788, NGC 2407 has a diameter of about 50,000 light-years. It is characterized by its bright core and well-defined spiral arms, making it an interesting object for astronomers studying galaxy formation and structure.