The galaxy presents as a somewhat elliptical structure, although exhibiting a moderate degree of roundness. The central region displays a bright, concentrated core that fades gradually outward. The overall color is a pale blue-white, suggesting the presence of intermediate stars. Subtle variations in color are noticeable, possibly indicating varying stellar populations. The lack of distinct spiral arms or a pronounced disk structure implies that it is potentially a lenticular or early-type spiral galaxy. No major or minor mergers are visually apparent, as the galaxy looks undisturbed.
