NGC 247 is a barred spiral galaxy located approximately 11 million light-years away in the constellation Cetus. It is part of the NGC 253 group of galaxies and is often referred to as the "Cetus Dwarf Galaxy." NGC 247 has a diameter of about 100,000 light-years and contains a significant amount of star formation activity. The galaxy is notable for its elongated shape and bright central bar structure. It is classified as a type SBc galaxy, indicating its spiral arms are loosely wound. Observations of NGC 247 have provided valuable insights into the formation and evolution of galaxies in the universe.