NGC 2452 is a planetary nebula located in the constellation Puppis. It is approximately 1,500 light-years away from Earth and is known for its bright central star, which is a remnant of a dying star that has shed its outer layers. The nebula has a distinct oval shape and exhibits a variety of colors due to the ionization of gases. Discovered by John Herschel in 1834, NGC 2452 is classified as a type of planetary nebula, which is a stage in the life cycle of certain stars. The nebula's structure is complex, featuring knots and filaments that provide insight into the processes of stellar evolution and the dynamics of gas ejection.