The galaxy presents as a centrally concentrated, somewhat spheroidal object. It exhibits a smooth, diffuse appearance with a gradual decline in luminosity from the core to the outer regions. There is a subtle color gradient, with the central region displaying a yellowish hue, suggesting an older stellar population, while the outer regions appear slightly bluer, potentially indicating the presence of younger stars or ongoing star formation. The overall structure lacks any prominent spiral arms or distinct features, indicating that it is likely an elliptical or lenticular galaxy, appearing relatively undisturbed. There may be some minor irregularities in the outer halo, but the overall morphology is largely smooth and undisturbed.