The galaxy presents as a spiral type, observed at an angle oblique to face-on. Two distinct spiral arms appear to emanate from a bright, moderately sized central bulge. The spiral arms exhibit a flocculent structure, with medium winding, tracing a generally symmetric pattern around the nucleus. The color gradient suggests ongoing star formation within the arms, with bluer hues indicative of younger stellar populations. There is no obvious bar structure bisecting the bulge. The dust lanes appear mottled. The galaxy displays no signs of tidal tails or significant morphological disturbances indicating recent major merger activity, though a minor disturbance cannot be ruled out.
