The galaxy presents an elliptical morphology, with a smooth, concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. The core region exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions show a subtle shift towards bluer tones, hinting at the presence of younger stars, but the overall color is still quite red. There are faint traces of disk structure, however it appears heavily obscured by dust. There is no obvious sign of tidal disturbances or other merger activity.
