The galaxy presents as an elliptical morphology with a high degree of smoothness. Its color index suggests a population of older stars and minimal on-going star formation. The galaxy displays a generally round appearance, with a slight deviation towards an intermediate shape. There is no apparent evidence of a major merger event or significant tidal disturbances; it's unlikely to be strongly interacting with any neighboring galaxies. The overall light profile is concentrated toward the center, fading gradually into the surrounding background. No prominent spiral arms or distinct structural features are discernible in this image.
