The galaxy presents as a somewhat elliptical, luminous entity with a concentrated central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population, while the outer regions appear fainter and slightly bluer. The lack of well-defined spiral arms or a distinct disk structure implies that this is likely an early-type galaxy, possibly an elliptical or lenticular. There are no obvious signs of recent or ongoing major mergers, although the faint outer regions hint at a possible past interaction or minor disturbance. The galaxy appears relatively smooth in texture, with a gradual decrease in luminosity from the center outwards.
