The galaxy presents as an edge-on spiral or lenticular system. It exhibits a flattened disk structure with a noticeable central bulge. The disk appears relatively smooth, with little evidence of prominent spiral arms or distinct dust lanes in this image, suggesting a more evolved or quiescent system. The color gradient across the galaxy indicates a potential difference in stellar populations, with the central bulge appearing yellower, indicative of older stars, and the disk exhibiting a slightly bluer hue, possibly indicating younger stars or ongoing star formation, however faint. The shape is significantly elongated, with an axial ratio suggesting it is close to being viewed perfectly edge-on. There is no apparent evidence of any major merger events or strong tidal distortions, suggesting that it is a relatively undisturbed galaxy.
