The galaxy presents as a spiral galaxy with a prominent, moderately sized bulge. The spiral arms are tightly wound and display a flocculent structure. Two spiral arms are clearly discernible. The disk is not viewed edge-on. There is no apparent strong bar structure, though a weak bar may be present. There is little to no evidence of a merger or major disturbance; the galaxy appears relatively undisturbed. The central bulge exhibits a yellowish hue, indicative of an older stellar population, while the spiral arms appear bluer, suggesting more recent star formation activity.
