The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology with a prominent bulge. It displays a relatively high degree of symmetry, with a noticeable elongation along its major axis. The central region exhibits a bright, condensed core, which appears to fade into a more diffuse halo.

Color gradients are subtle but present. The central bulge appears bluer compared to the outer regions, which tend towards redder hues. This suggests a difference in stellar populations, with the core possibly hosting younger, hotter stars and the outer regions dominated by older, cooler stars.

There's little evidence of strong tidal features or disturbances, suggesting a relatively quiescent evolutionary history. However, there is a slight asymmetry in the isophotes within the halo region, indicating possible past interactions.
