This galaxy presents as a relatively face-on spiral, exhibiting a disk structure with notable spiral arm features. The spiral arms are somewhat loosely wound and possess a patchy, flocculent appearance, indicating regions of active star formation. These regions are characterized by a bluish tint, consistent with the presence of young, hot stars. The central bulge is not very prominent, appearing relatively small and not sharply defined. There is a suggestion of a bar-like structure bisecting the central region, although it does not appear to be a particularly strong or well-defined bar. There is evidence of some degree of interaction or disturbance in the overall morphology, with some asymmetry and possible tidal features hinted at, perhaps suggesting minor gravitational interactions. Overall, it appears to be a spiral galaxy with ongoing star formation, a relatively small bulge, and possibly influenced by a recent interaction.
