NGC 2405 is a spiral galaxy located in the constellation Camelopardalis. It is approximately 100 million light-years away from Earth and is part of the Hubble Space Telescope observations, which have provided detailed images of its structure. This galaxy is notable for its bright core and well-defined spiral arms, which are characteristic features of spiral galaxies. NGC 2405 is also classified as a member of the Leda database, which catalogs various astronomical objects, helping astronomers study its properties and behavior in the universe.