The galaxy appears as an elongated, somewhat spindle-shaped structure, suggesting it is likely an edge-on spiral or a lenticular galaxy. It has a central bulge that appears relatively smooth and concentrated, displaying a yellowish hue, possibly indicating an older stellar population. The disk component, extending outwards from the bulge, shows a faint bluish tint, implying the presence of younger, hotter stars and ongoing star formation. The galaxy's overall structure seems relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There are faint hints of dust lanes running along the disk, but without higher resolution it is hard to be certain. Its elongated shape suggests a dynamically stable system with a significant rotational component. The size appears modest, consistent with it being a typical galaxy in the distant universe.
