The galaxy presents as a centrally concentrated object, consistent with an elliptical morphology or a bulge-dominated spiral galaxy. The light profile appears smooth, lacking any distinct spiral arm structures or prominent dust lanes. Its shape is elongated, indicating a deviation from perfect circularity. The galaxy exhibits a relatively uniform color distribution across its visible extent. The galaxy's apparent size suggests it is a relatively large object, and the relatively well-defined edge indicates it is not likely to be currently undergoing a major merger event, although minor disturbances are not ruled out.
