This galaxy exhibits a clear spiral structure. The spiral arms are tightly wound around a prominent central bulge. A bar appears to traverse the bulge region. The bulge itself seems moderately sized, and its luminosity suggests a significant population of older stars. The spiral arms display a granular texture, indicative of active star formation regions. The colors observed within the arms suggest a population of young, hot stars interspersed with dust lanes. The overall morphology suggests a relatively undisturbed system with well-defined spiral structure, though some asymmetry is noticeable. A moderate amount of light can be seen around the main body of the galaxy. The galaxy is not viewed edge-on; rather, it is at an angle that allows clear observation of the disk's features. It is most likely not a merging or disturbed galaxy.
