The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. The core region exhibits a strong yellow hue, likely indicating an older stellar population and reduced star formation. The outer regions of the galaxy show a gradual decline in luminosity, transitioning to a more reddish color. This suggests the presence of evolved stars and dust. There are subtle indications of tidal disturbance but they are minor. The overall structure appears relatively undisturbed, exhibiting no strong signs of ongoing major mergers or significant morphological peculiarities. The elongation hints at a potential disklike structure, though the smoothness may obscure any defined spiral arms.
