The galaxy presents a spiral morphology, with a noticeable central bulge. The spiral arms are tightly wound and exhibit a flocculent structure, lacking distinct, continuous features. There is a strong amount of dust and gas visible, especially throughout the arms. There are various star forming regions throughout the spiral arms. The galaxy does not appear to be significantly disturbed or undergoing a major merging event. The central bulge appears relatively small compared to the overall size of the disk. Overall, this spiral galaxy seems relatively well defined.
