The galaxy presents as a relatively smooth, centrally concentrated object with a subtly elongated shape. It exhibits a somewhat diffuse appearance. The core region appears brighter and more compact than the outer regions. The color profile appears homogenous, with a bias towards warmer, redder hues throughout the galaxy's structure. There is a hint of asymmetry to the overall structure, which suggests possible past interaction or internal dynamics affecting its morphology. No clear spiral arm structures or dust lanes are discernible. The galaxy appears undisturbed.
