NGC 6949 is a spiral galaxy located in the constellation Cepheus. It is approximately 22 million light-years away from Earth and is classified as a type Sc spiral galaxy, characterized by its well-defined spiral arms and a bright central bulge. Discovered by the astronomer William Herschel in 1788, NGC 6949 contains a significant number of young, hot stars, which contribute to its bright appearance. The galaxy is also known for its active star formation regions, making it an interesting subject for astronomers studying the processes of galaxy evolution and stellar birth.