The galaxy presents as a spiral type, with a prominent central bulge that appears elongated in the north-south direction. Faint spiral arms are visible extending outwards from the central bulge, displaying clumpy regions suggestive of active star formation. The overall color of the galaxy appears bluish-white, particularly in the spiral arms, which likely indicates the presence of a younger stellar population. There is evidence of some distortion in the galaxy's morphology. One side of the galaxy appears stretched or disrupted.
