The galaxy presents as a moderately bright, yellowish-orange elliptical galaxy. It exhibits a relatively smooth morphology, with no prominent spiral arms or distinct features visible. The galaxy appears somewhat elongated, though not extremely so, with an approximate axis ratio indicating it is closer to a circular shape than a highly flattened one. The color profile suggests an older stellar population dominating its light emission, consistent with a low star formation rate. There is a possibility of a minor interaction or disturbance based on the slight asymmetry observed in the outskirts of the galaxy, but the primary structure remains largely undisturbed. The overall appearance suggests a mature galaxy, likely having undergone significant evolutionary processes.
