The galaxy exhibits a generally smooth morphology, with a dominant elliptical shape. The light profile suggests a centrally concentrated structure. Its color is predominantly yellowish-orange, implying a relatively older stellar population with a lower rate of ongoing star formation. There are no immediately apparent spiral arms or significant dust lanes. The overall appearance indicates a mature galaxy, likely nearing the end of its star-forming period. Based on the shape, it is likely an elliptical galaxy. There is no evidence to suggest any ongoing major merging events or significant tidal disturbances.
