The galaxy exhibits a clear spiral morphology, with a dominant disk structure. The spiral arms are well-defined and possess a somewhat flocculent, patchy appearance. There are two dominant spiral arms. The arms appear moderately wound, not tightly compressed, and not very loosely wound. The central bulge is small relative to the disk size. A bar is present, extending through a good portion of the galaxy. There is little evidence of significant interaction or merging events, with only slight irregularities detected. There are few signs of distinct features within the disk. The color gradient suggests ongoing star formation.
