NGC 675 is a barred spiral galaxy located in the constellation Phoenix. It is approximately 70 million light-years away from Earth and is part of the Hubble Space Telescope catalog of galaxies. NGC 675 has a bright central bar structure, which is characteristic of barred spiral galaxies, and it exhibits a well-defined spiral arm pattern. The galaxy spans about 100,000 light-years in diameter, making it similar in size to our own Milky Way galaxy. NGC 675 is notable for its active star formation regions, which contribute to its bright appearance in optical wavelengths. Observations of this galaxy help astronomers understand the dynamics and evolution of spiral galaxies.