The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with no discernible spiral arms or disk structure. The light profile appears centrally concentrated, with the brightest region located at the core of the galaxy. The color gradient suggests the presence of an older stellar population, as the central region exhibits a yellowish-orange hue, while the outer regions appear slightly bluer. There is no obvious evidence of active star formation or dust lanes. The galaxy appears isolated, with no obvious signs of recent mergers or tidal disturbances. The object has a small angular size, giving it a nearly circular appearance.
