The galaxy exhibits a clear spiral structure. Two prominent spiral arms are visible, tightly wound around a central bulge. The bulge appears moderate in size. The overall color profile suggests ongoing star formation within the spiral arms, with bluer hues intermixed with the yellower light of older stellar populations. The galaxy is not viewed edge-on. There is no evidence of a strong bar structure. There is no obvious indication of a major merger event, though the spiral arms display some irregularities.
