The galaxy exhibits a spiral morphology, with loosely defined spiral arms extending from a central bulge. The arms appear somewhat patchy, indicating regions of active star formation. The central bulge has a moderate size, appearing relatively smooth and concentrated. The overall color suggests a mix of stellar populations, with bluer regions corresponding to younger stars in the spiral arms and a more yellowish hue in the bulge, indicative of older, redder stars. The galaxy appears tilted with respect to our line of sight, providing a partial view of the galactic disk. There is no immediately noticeable evidence of a strong bar structure or major merging activity, though minor disturbances cannot be ruled out from this image alone. The disk appears to be fairly well-defined, with a slightly flattened shape.
