NGC_5005 is a spiral galaxy located approximately 24 million light-years away in the constellation Canes Venatici. It is classified as a type SA(s)c galaxy, which means it has a well-defined spiral structure and is actively forming new stars. The galaxy is notable for its bright core and prominent spiral arms, which are rich in young, hot stars. NGC_5005 is often studied by astronomers to understand the processes of star formation and the dynamics of spiral galaxies in the universe.