The galaxy appears to be a spiral galaxy, exhibiting distinct spiral arms. These arms are somewhat loosely wound and appear to be actively forming stars, as evidenced by the patchy blue regions distributed along their length. The central bulge region is prominent, displaying a yellowish color, which suggests an older stellar population. The galaxy's disk is not perfectly face-on, but rather appears to be inclined slightly. There is evidence of a possible bar structure crossing the central bulge, although it is not highly pronounced. The galaxy appears to be undergoing some form of interaction or disturbance as there are some asymmetries in the disk structure, particularly at the ends of the arms. The overall appearance suggests a galaxy with ongoing star formation, a moderately sized bulge, and possibly some recent or ongoing interaction influencing its morphology.
