The galaxy presents as an elliptical-like object with a smooth, centrally concentrated light distribution. It exhibits a moderate ellipticity, appearing somewhat elongated, but not distinctly disk-like. The central region appears brighter and more compact than the outer regions. There is some subtle visual evidence of faint, diffuse structure or possible tidal features extending away from the main body of the galaxy, suggesting a potential interaction or minor disturbance, although it is difficult to state with certainty. The overall color is consistent with a more evolved stellar population.
