The galaxy presents as a largely smooth, elliptical morphology. The central region exhibits a high degree of luminosity and is slightly oblong in shape. Moving outwards, the light gradually decreases. The main body of the galaxy does not appear to have any visible spiral arm structures or dust lanes. There may be a slight asymmetry on one side which might be interpreted as a possible tidal feature, though it is not prominent. The overall color is more consistent with a population of older stars as evidenced by the yellowish hue. It shows no indications of recent major merging events or significant disk formation. The galaxy appears relatively isolated.
