The galaxy presents as a spiral type. A central bulge is observable but not highly pronounced. Two prominent spiral arms appear to originate near the core region and loosely wind outward. Patches of higher luminosity are observed within the spiral arms, consistent with areas of active star formation. The bluer color of the arms indicates a stellar population with higher temperatures, consistent with star formation regions. The central bulge has a slightly reddish hue, suggesting an older, cooler stellar population. The galaxy does not appear to be strongly barred. There is no clear sign of recent or ongoing merger activity. The overall structure is well-defined.