The galaxy presents as a largely featureless elliptical type. Its color profile indicates a central concentration of older stellar populations, appearing yellowish-orange in the composite image. The galaxy exhibits a smooth light distribution with minimal discernible substructure. The overall shape is somewhat elongated, but not highly so, appearing closer to elliptical than a highly flattened disk. There is no visually apparent evidence of a major ongoing merger event or significant tidal disturbances. It appears to be a relatively undisturbed system.
