The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. A slight elongation is observed, suggesting a deviation from a perfectly circular form. The light distribution is centrally concentrated with a gradual decrease in intensity outwards, creating a diffuse halo. Coloration suggests an older stellar population, exhibiting primarily yellow-orange hues. There is no prominent dust lane or spiral arm structure visible. The galaxy shows no apparent signs of on-going major mergers or significant tidal disturbances, but might be experiencing minor disturbances.