The galaxy appears to be an edge-on spiral galaxy at a moderate redshift. It presents a distinctly flattened disk structure. A prominent central bulge is visible, exhibiting a smooth, rounded morphology and concentrated luminosity. The disk component is noticeably thinner than the bulge, with some faint dust lanes visible. Overall, the galaxy appears relatively undisturbed, showing no signs of recent major merger activity or significant tidal interactions. The galaxy exhibits a color gradient, with the bulge appearing redder, indicating an older stellar population. The disk shows bluer hues suggesting ongoing or recent star formation.
