The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish-white hue, suggesting the presence of an older stellar population. The galaxy's light gradually fades outwards from the core. There is little evidence of spiral arm structure or distinct features, supporting the classification of a smooth galaxy. Faint extensions are slightly present but not clearly defined suggesting possible tidal disturbances. Overall, the galaxy appears relatively undisturbed with a high degree of symmetry.
