The galaxy presents a distinct spiral morphology. Spiral arms are prominent, winding moderately around a central bulge. The arms show a complex structure, with indications of varying stellar densities and potential star formation regions, as suggested by the somewhat patchy distribution of light. The galaxy appears to exhibit a substantial disk component, with a moderate bulge. There is a suggestion of multiple spiral arms. The system does not show strong evidence of major mergers or significant disturbances, though minor disturbances may be present. The central bulge is not dominant, but it does possess a definite presence. Some of the spiral arms are tightly wound, while others show a more open structure.
