NGC 4395 is a unique and intriguing galaxy located in the constellation Canes Venatici, approximately 14 million light-years from Earth. Unlike many well-known galaxies, NGC 4395 is classified as a low surface brightness galaxy and lacks the prominent spiral arms that characterize more typical spiral galaxies. Its diffuse and irregular appearance makes it an interesting subject of study, particularly for understanding the variety of galactic structures and formations in the universe.

One of the most remarkable features of NGC 4395 is its low-mass central black hole, estimated to be around 10,000 times the mass of the Sun. This black hole is one of the smallest supermassive black holes known, providing valuable insights into the lower end of the supermassive black hole mass spectrum and its impact on the host galaxy. NGC 4395 also exhibits active galactic nucleus (AGN) activity, emitting X-rays and ultraviolet light, which offers a unique opportunity to study the relationship between black holes and galaxy formation in environments with minimal stellar activity.