NGC 7219 is a barred spiral galaxy located approximately 60 million light-years away in the constellation Camelopardalis. It was discovered by the astronomer John Herschel in 1827 and is classified as a type SBc galaxy, indicating its spiral structure with a central bar. The galaxy has an apparent magnitude of about 13.5, making it faint and challenging to observe with small telescopes. NGC 7219 is part of a group of galaxies and is of interest to astronomers studying galaxy formation and evolution due to its distinct features and structure.