The galaxy presents as a luminous, relatively smooth object with a concentrated central bulge. The light distribution suggests a near-spherical, rather than disk-like, morphology. There is a radial color gradient apparent, transitioning from a yellowish-white core to a more reddish, diffuse outer halo. While the object is primarily smooth in appearance, there are subtle indications of possible minor disturbances in the outer regions, without any prominent signs of mergers. The galaxy displays a round profile, lacking any distinct elongation or asymmetry. Overall, the appearance indicates a system dominated by older stellar populations.
