The galaxy presents as a spiral structure with a moderate inclination relative to our line of sight. The central bulge exhibits a concentrated luminosity, appearing relatively smooth and yellowish in color. Faint arms can be seen extending from the central region and are tightly wound. The galaxy exhibits a disk-like morphology, with some irregularity in the outer regions suggesting possible interactions or internal disturbances. The spiral arms are primarily composed of young, hot stars. There is no evidence of a strong bar structure in the galaxy's center.
