The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a yellowish-white hue, suggesting a population of older stars. A fainter, bluish halo surrounds the central region, potentially indicating younger stellar populations or regions of ongoing star formation. The galaxy appears relatively undisturbed, lacking any obvious signs of tidal interactions or major mergers. Its overall color indices imply a significant presence of evolved stars, consistent with a relatively low specific star formation rate. The galaxy's light distribution follows a fairly concentrated profile, with the outer regions gradually fading into the background. It appears somewhat flattened along its minor axis, resulting in an elongated appearance.
