This galaxy exhibits a prominent spiral structure. The spiral arms appear tightly wound, emanating from a distinct central bulge. The bulge appears moderate in size relative to the overall galactic disk. The galaxy is viewed at an angle, somewhere between face-on and edge-on. The nucleus is bright and centrally concentrated. Colors suggest a mixture of stellar populations, with bluer regions potentially indicating areas of recent star formation within the spiral arms. There is no obvious evidence of a strong bar structure or major mergers. There may be slight disturbances or asymmetries visible in the outer disk, potentially hinting at minor interactions.
