The galaxy presents as an edge-on spiral. A prominent bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population and reduced star formation in the galactic center. The disk appears relatively thin and elongated, displaying a bluish tint that may indicate the presence of younger, hotter stars and ongoing star formation. The outer regions of the disk fade into the background sky, with the dust lane not visible based on the image, the spiral arms also cannot be seen. The light distribution appears smooth and without any obvious signs of major disturbances or mergers.
