The observed galaxy presents as a highly elongated, edge-on spiral. There is a prominent central bulge exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk appears relatively smooth, lacking distinct spiral arm structures. The outer regions of the disk show a subtle blue tinge, indicative of recent star formation. The galaxy's overall morphology is suggestive of a system with a considerable stellar mass. There's no obvious visual indication of any major ongoing merger events, but the smoothness of the disk could indicate a previous interaction.
