The galaxy presents as a spiral type, exhibiting a disk-like structure. The spiral arms appear loosely wound, with a suggestion of two dominant arms visible. Patches of concentrated light suggest active star-forming regions within the arms. The central bulge seems relatively small compared to the overall disk size, possibly indicating a lower mass concentration in the nucleus. Evidence suggests a major disturbance or possible merger event, evidenced by the galaxy's asymmetric form. There is a tidal tail visible, which is a sign of gravitational interaction. Overall color indices suggest moderate star formation activity and likely the presence of a stellar population spanning a range of ages. 
