NGC 2403

NGC 2403 is a spiral galaxy located approximately 8 million light-years away in the constellation Camelopardalis. This galaxy is notable for its active star formation regions, evident in the bright H II regions scattered throughout its arms. Observers can also find numerous star clusters and supernova remnants, which add to its visual appeal. NGC 2403 is a delightful target for amateur astronomers and astrophotographers alike, providing a rich field of study in the realm of galactic evolution and structure.