The galaxy presents a primarily smooth morphology, appearing elliptical in shape with a high degree of roundness. There is a concentration of light towards the center, suggesting a prominent bulge. The color is predominantly yellow, which indicates an older stellar population with limited ongoing star formation. Subtle hints of a disc structure may be present; however, the smoothness dominates the overall appearance. There is no clear evidence of a major merger or significant tidal disturbances. Subtle irregularities may be visible, which could suggest minor disturbances, but the overall symmetry and lack of pronounced features indicate a relatively undisturbed system.
