A type of spiral galaxy first discovered by U.S. astronomer, Karl Seyfert (1911-1960), in the 1940s: The central region of a Seyfert galaxy is distinguished by powerful radiation, much of it is focused into narrow frequencies.

A Seyfert galaxy is a galaxy with an unusually bright central nucleus, often emitting strongly in the infrared region of the electromagnetic spectrum, as a result of hot dust within it.

About two per cent of all galaxies are Seyfert galaxies.

A Seyfert galaxy can be desccribed as a spiral galaxy with a small, compact, bright nucleus that exhibits variable light intensity and radio-wave emission.