The galaxy presents a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The light distribution is concentrated towards the center, exhibiting a high degree of radial symmetry. The galaxy has an overall rounded shape. Color gradients suggest a population of older stars, with a yellowish hue dominating the central region, indicating a potentially low rate of current star formation. There is no visual indication of a major ongoing merger or significant tidal disturbance.
