NGC 1894 is a globular cluster located in the constellation of Lepus. It is approximately 50,000 light-years away from Earth and contains a large number of stars, estimated to be around 100,000. This cluster is notable for its relatively high concentration of stars in a small area, making it a fascinating object for astronomers. Discovered by William Herschel in 1785, NGC 1894 is classified as a type of globular cluster, which are spherical collections of stars bound together by gravity. These clusters are typically older and can provide insights into the early formation of the Milky Way galaxy.