NGC 7225 is a spiral galaxy located approximately 50 million light-years away in the constellation Pegasus. It is part of a group of galaxies known as the NGC 7225 group, which includes several other galaxies and is notable for its interactions and gravitational influences. This galaxy has a diameter of about 50,000 light-years and is characterized by its bright core and well-defined spiral arms. NGC 7225 is also classified as a type Sc spiral galaxy, indicating a specific structure and star formation activity within its arms.