NGC 4692 is a barred spiral galaxy located in the constellation Centaurus. It is approximately 150 million light-years away from Earth and is part of the Centaurus Galaxy Cluster. This galaxy is notable for its bright core and well-defined spiral arms, which contain numerous stars and regions of active star formation. NGC 4692 is also classified as a Seyfert galaxy, indicating that it has an active nucleus that emits significant radiation, often due to the presence of a supermassive black hole at its center.