The galaxy presents as a spiral type, exhibiting a clear disk structure. Two well-defined spiral arms are the dominant feature. These arms appear tightly wound near the central bulge and gradually loosen as they extend outwards. A central bulge is quite pronounced, displaying a smooth, concentrated luminosity. A bar-like structure is visible cutting through the central bulge, appearing strong and well-defined. The overall orientation of the galaxy is neither face-on nor edge-on but presented at an intermediate angle. The disk shows a slight inclination. There is evidence of ongoing star formation, particularly within the spiral arms, indicated by subtle variations in color and luminosity. No signs of major disturbances or recent mergers are immediately apparent, but a minor asymmetrical feature on one edge of the galaxy suggests possible tidal interaction. The central bulge appears relatively large, and the galaxy presents with a large amount of mass.