The galaxy presents as a relatively smooth, elliptical-like structure. Its color is predominantly orange/yellow, suggestive of an older stellar population. A central, brighter region is visible, potentially indicating a galactic bulge. The galaxy exhibits a moderate degree of elongation. Faint extensions are observed, appearing to be very minor tidal disturbances or possible faint spiral arms. There are no prominent dust lanes visible, which is consistent with it being an elliptical galaxy. The overall form is relatively undisturbed, indicating it has not undergone a major merger recently. It is likely to be a relatively massive system with intermediate star formation occurring.
