The galaxy presents as a largely smooth, elliptical morphology. Its light profile appears concentrated towards the center, indicating a prominent bulge. The core region exhibits a yellow-white hue, suggesting an older stellar population. Fainter, bluer light surrounds the core, potentially indicating some ongoing or recent star formation. The galaxy does not display any prominent spiral arms or a distinct disk structure, and there's no apparent sign of tidal tails or strong morphological disturbances that would indicate a recent major merger event. There is only a minor possible disturbance within the galaxy. Overall, the galaxy seems to be a relatively undisturbed system with an intermediate redshift.