The galaxy appears to be a spiral galaxy viewed at a moderate inclination. Two spiral arms are clearly visible, with a loosely wound morphology. The arms display clumpy regions, which may be areas of active star formation. The central bulge is moderately prominent and appears yellowish, potentially indicating an older stellar population. There is no sign of a prominent bar structure. The overall color suggests the presence of both young and old stars. There is no evidence of any major merger event. The arms are somewhat symmetric, suggesting a relatively undisturbed morphology.
