The galaxy exhibits a clear spiral structure with well-defined arms. The arms appear flocculent, with some winding more tightly than others. A central bar structure is strongly present, bisecting the galaxy's core. The core displays a moderate bulge size, neither dominating the disk nor appearing insignificant. The disk is oriented approximately face-on. The arm count indicates at least two to four distinct spiral arms are visible. There's no strong indication of a major merger event, although some minor irregularities may be present. The galaxy's color profile suggests a mix of stellar populations, with bluer regions associated with the spiral arms and a slightly redder central bulge. The overall form is fairly regular, though some patchiness is observed in the arms.
