The galaxy appears as a centrally concentrated elliptical. Its overall color profile indicates a redder population, suggesting an older stellar population, with minimal recent star formation. The galaxy presents a smooth and largely featureless morphology, displaying a high degree of rotational symmetry. There is no apparent dust lane, spiral arm structure, or tidal disturbance indicating a recent major merger event. Faint, extended light suggests a diffuse halo surrounding the central region. The morphology is generally consistent with an early-type galaxy, likely an elliptical.
