The galaxy exhibits a discernible disk structure. Two spiral arms appear to emanate from the central bulge, with a moderate winding. The arms display a degree of patchiness suggesting regions of star formation. The central bulge appears moderately prominent, and slightly elongated. The galaxy's color suggests ongoing star formation, though the bulge exhibits a more yellow-red hue, potentially indicative of an older stellar population. There is no obvious major disturbance to the overall morphology indicative of recent major merger activity. The disk of the galaxy is not oriented edge-on.
