This galaxy exhibits a distinct spiral structure. The spiral arms are tightly wound and numerous. There is a prominent central bulge, surrounded by a disk that appears to be viewed at a slight inclination. The arms appear to be composed of a mix of star formation regions and older stellar populations. Evidence suggests that a significant proportion of the galaxy's light originates from the disk component. There is no obvious sign of major ongoing mergers or tidal disturbances. The spiral arms are relatively symmetric around the bulge, indicating a dynamically relaxed system.
