The galaxy appears as a highly elongated, edge-on spiral system. A prominent central bulge dominates the structure, appearing smooth and relatively featureless. There is a distinct color gradient along the galaxy's major axis, with the central bulge exhibiting a yellowish-orange hue and the outer disk regions displaying a more blue-ish tint. The disk itself appears relatively thin and exhibits a smooth, diffused light distribution, likely due to dust obscuration and potentially indicating a relatively quiescent star formation rate. No clear spiral arm structure is discernible. The galaxy seems undisturbed, with no visible signs of recent mergers or interactions.
