NGC 1672 is a barred spiral galaxy located approximately 60 million light-years away in the constellation Dorado. It is notable for its prominent bar structure and well-defined spiral arms, which are characteristic features of this type of galaxy. Discovered by the astronomer John Herschel in 1835, NGC 1672 has a diameter of about 100,000 light-years. It is classified as a Seyfert galaxy, indicating that it has an active nucleus with bright emissions, often associated with a supermassive black hole at its center.