The galaxy presents a distinct spiral morphology. It exhibits a prominent, moderately sized central bulge that appears bright and yellowish in color, indicative of an older stellar population. Surrounding the bulge are well-defined spiral arms, wound tightly around the galactic center. The arms display a clumpy structure, suggesting ongoing star formation. These regions are bluer in color, consistent with the presence of young, hot stars. Indications of a bar-like structure exist within the inner region of the galaxy. There appears to be no obvious signs of major merging activity, but the spiral arms are somewhat asymmetrical.
