The object is a spiral galaxy viewed nearly edge-on. A prominent central bulge is visible, appearing a yellow-white hue, indicating an older stellar population. The disk is relatively smooth and appears to have faint spiral arm structures, with subtle differences in color suggestive of ongoing star formation regions, although these are not well-defined. The galaxy is likely relatively massive, but exhibiting a low star formation rate. There is no strong indication of a recent or ongoing major merger event.
