The galaxy presents as an edge-on spiral system. A prominent central bulge appears yellowish-white, suggesting an older stellar population concentrated towards the core. The disk is elongated and thin, displaying a mottled bluish hue on both sides of the bulge that fades away as it gets further away from the center, which may indicate ongoing star formation within the spiral arms. The disk appears relatively smooth, with no obvious signs of major disturbances or merger events. There's a subtle warping of the disk, and it appears slightly lopsided with one side of the disk being slightly brighter.
