The galaxy exhibits a spiral morphology, with prominent arm structures emanating from a central bulge. The arms appear to be tightly wound in some areas and moderately open in others. Two main spiral arms are clearly visible. The disk of the galaxy presents a slightly tilted aspect relative to our line of sight, implying it is neither perfectly face-on nor edge-on. A bar-like structure appears to traverse the center of the galaxy. The light distribution suggests a moderate-sized central bulge relative to the disk. No significant signs of ongoing major mergers are observed, though some minor disturbances within the disk might indicate recent interactions. The galaxy displays a smooth, centrally concentrated brightness profile, with colors indicating active star formation regions, though it is likely undergoing quenching.
