The galaxy exhibits a clear spiral structure, although the arms are not sharply defined. A prominent central bulge dominates the galaxy's core, appearing somewhat brighter and more concentrated than the surrounding disk. The spiral arms appear flocculent with medium winding, with some arms appearing more prominent and well-defined than others. Dust lanes are faintly visible within the spiral arms, adding to the complexity of the structure. There is a hint of a bar structure spanning the central bulge. The disk component appears relatively flat and extends outwards from the central bulge. Star formation regions are present, with areas appearing bluer in color. No major merging events are detected, though there could be some minor disturbances present in the spiral arm morphology. The overall color of the galaxy suggests a mix of stellar populations.
