The galaxy presents as a somewhat elliptical, well-defined object with a smooth appearance, indicating a likely classification as an elliptical galaxy. Its core exhibits a concentrated, bright yellowish-orange hue, suggesting an older stellar population dominating the central region. Progressing outwards from the core, there is a gradual shift to a more greenish color. This suggests a possible presence of younger stars or a different stellar population in the outer regions, though the smoothness implies no recent major merger activity that would disrupt the overall morphology. No distinct spiral arms or prominent dust lanes are visible, further supporting the elliptical classification. There are no signs of major tidal disturbances or ongoing merger events. The galaxy appears relatively isolated and undisturbed, with its shape and color gradients suggesting a stable and evolved system. 
