The galaxy presents as a spiral type, characterized by a prominent central bulge that appears relatively bright and moderately sized in comparison to the disk. The disk component exhibits a notable presence of spiral arm structures. These arms are somewhat loosely wound and display a patchy, flocculent appearance, suggesting regions of active star formation. There is a distinct blue hue within the spiral arms, indicative of a population of young, hot stars. The overall morphology suggests ongoing, but perhaps not extremely intense, star formation activity. No significant signs of tidal disturbance or major merging events are apparent, although minor irregularities within the disk could suggest past interactions. The galaxy's orientation allows for a face-on view, aiding in the observation of its spiral structure. A faint bar-like structure can not be excluded but is difficult to identify, with an oval-shaped structure instead appearing.
