The galaxy presents a generally smooth and elliptical morphology, with a concentrated central bulge. The overall color is consistent with an older stellar population, appearing yellowish-orange. The lack of discernible spiral arms or patchy blue regions suggests a relatively low rate of ongoing star formation. There is a hint of asymmetry, indicating a possible past interaction or merger. No significant dust lanes are visible. The light distribution indicates that this is a large and massive galaxy. There is a low probability of the galaxy being a merger based on these morphological features.