The galaxy presents as a spiral morphology, exhibiting well-defined spiral arms. These arms appear to be relatively tightly wound around a prominent central bulge. The bulge displays a concentrated luminosity, indicating a high density of stars and/or a potential supermassive black hole at the galactic center. The spiral arms show a bluer color, suggesting ongoing star formation within these regions. Dust lanes are visible within the spiral arms, obscuring some of the light emitted from the stars behind them. There is a potential indication of a bar structure bisecting the central bulge, although the resolution of the image makes it somewhat difficult to confirm with certainty. The disk component appears relatively smooth and unperturbed. The overall structure suggests a relatively undisturbed and mature spiral galaxy.