The galaxy presents as a spiral type, exhibiting distinct, though somewhat blurred, spiral arm structures. These arms appear to be tightly wound around a central bulge. The spiral arms are a blueish hue, suggesting active star formation. The central bulge appears less defined, and relatively small. There is no apparent bar structure. There is no visual evidence of a major merger, but there may be some minor disturbances to the symmetry of the spiral arms. The galaxy appears to have at least two spiral arms.