The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse appearance. There is a distinct color gradient, transitioning from a yellowish-orange core to fainter, redder outer regions. No distinct spiral arms or features are visible. The morphology suggests a relatively evolved system with a predominantly older stellar population. The light distribution indicates a high degree of symmetry. There is a possibility of very subtle asymmetries, but they are within the errors of the image quality. Based on these features and estimated distance, this is a moderate-sized galaxy with very low star formation rates, suggesting most star formation occurred long ago.
