The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge. Its overall color gradient indicates a relatively uniform stellar population, with a yellow-white hue near the core, indicative of older stars. There is a subtle color shift to bluer tones in the outer regions which may indicate some, but not extensive, younger star formation. No spiral arm structures or significant dust lanes are discernible. The galaxy shows a high degree of circularity. There is no apparent tidal distortion or any signs of ongoing mergers.
