The galaxy presents a largely featureless, elliptical morphology. It appears to be a relatively smooth object, with a high degree of central concentration. The light distribution exhibits a radial gradient, with the core displaying a brighter, more intense emission, trending towards a more diffuse halo. There is a slight color gradient, with the central region appearing more yellow-white, suggesting an older stellar population, and the outer regions appear to be a more dull blue, suggesting a slightly younger stellar population in the halo. Overall, the galaxy appears undisturbed, showing no signs of recent merger activity or tidal distortions.
