This galaxy exhibits a clear disk-like structure, oriented nearly edge-on from our line of sight. The central region presents a higher concentration of light, appearing yellowish-white, suggesting an older stellar population. This central bulge is prominent and elongated.

The disk shows a bluer hue, particularly towards the edges. Irregular patches of light and dark areas along the disk's outer edges are observed. These could indicate regions of star formation and dust lanes, respectively. The overall structure seems relatively undisturbed, with no obvious signs of a major merger or strong tidal interactions.
