The galaxy presents as an elliptical or lenticular morphology, appearing largely smooth and featureless. The central region exhibits a strong concentration of light, suggesting a prominent galactic bulge. A color gradient is discernible, transitioning from a yellowish-orange core to a slightly bluer halo region, which may indicate a difference in stellar populations, with older, redder stars dominating the center and younger, bluer stars possibly present in the outer regions, although this could also be influenced by dust content. There are slight asymmetrical distortions, possibly indicative of tidal interactions or minor disturbances in the gravitational potential, but there is no strong evidence of a major ongoing merger. The overall appearance is that of a relatively evolved system.
