NGC 1964

NGC 1964 is a barred spiral galaxy located in the constellation Lepus. It was discovered on November 20, 1784, by William Herschel.

NGC 1964 is estimated to be approximately 200 million light-years away from Earth. Its apparent magnitude is around 11.9, making it visible through moderate-sized telescopes.

The galaxy is classified as an SB(rs)b type galaxy, indicating that it is a barred spiral galaxy with a weak ring structure and moderately tightly wound spiral arms. The "SB" designation indicates the presence of a bar-shaped structure in the center, which is a common feature in many spiral galaxies. The "(rs)" portion indicates a weak inner ring structure around the bar. The "b" designation refers to the tightness of the spiral arms, with "b" indicating moderately tightly wound arms.

Studies of NGC 1964 have contributed to our understanding of galaxy morphology, spiral arm formation, and the distribution of matter in the universe. Its distance and redshift measurements are used in cosmological studies.