The galaxy exhibits a well-defined spiral structure. The arms appear flocculent, displaying a patchy distribution of star formation regions. The spiral arms are tightly wound around a central bulge. The bulge is moderately prominent, appearing somewhat bright. The galactic disk is oriented approximately face-on relative to our line of sight. There is no obvious indication of ongoing major merging activity, although subtle disturbances within the disk cannot be ruled out. The galaxy's overall color suggests a mix of stellar populations, including both younger, bluer stars within the spiral arms and older, redder stars in the bulge.
