The galaxy presents a distinct spiral morphology, exhibiting prominent, loosely wound spiral arms. The arm structure is somewhat flocculent, displaying clumpy regions indicative of active star formation. The arms emanate from a moderately sized central bulge region, showing a clear disk inclination, as it is seen from an angle that is not face-on. There is evidence of a possible bar structure across the central region, slightly elongated.

The overall color suggests recent star formation, indicated by the bluer hues in the spiral arms. Areas of disturbance and asymmetry are observed, which may suggest interaction with a companion galaxy or recent merger activity.
