NGC 4214 is an irregular galaxy located in the constellation Canes Venatici, approximately 10 million light-years from Earth. This galaxy is characterized by its chaotic structure, lacking the defined spiral arms or elliptical shape seen in more regular galaxies. NGC 4214 is a prolific star-forming region, with numerous bright star clusters and massive young stars scattered throughout its irregular form.

One of the notable features of NGC 4214 is its large H II regions, where intense star formation is occurring. These regions are illuminated by the ultraviolet light from young, hot stars, causing the surrounding hydrogen gas to glow brightly. Observations have revealed that NGC 4214 contains both young and old stellar populations, making it an excellent laboratory for studying the processes of star formation and galactic evolution. The galaxy's irregular shape and active star-forming regions provide valuable insights into the dynamics and history of irregular galaxies.