The galaxy presents as a centrally concentrated spheroid with a smooth, featureless appearance. Its morphology suggests an evolved system, lacking prominent spiral arms or significant dust lanes. The color profile indicates a dominant older stellar population, with a yellowish-orange hue concentrated in the central region, suggestive of a high concentration of evolved stars. There is a subtle extension of redder emission towards the periphery. The overall shape is close to circular, with only slight deviations from perfect radial symmetry, although some asymmetry is present. There is no obvious evidence of a strong tidal interaction or ongoing major merger event, but very minor disturbances cannot be ruled out.
