The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. Its shape is elongated, displaying a ratio of the semi-minor to semi-major axis of approximately 0.65. There's a noticeable color gradient, with the central region appearing more yellow/white and shifting to a slightly redder hue in the outer regions. This color gradient potentially indicates varying stellar populations, with older stars dominating the core. The lack of discernible spiral arms or dust lanes suggests a relatively quiescent star formation history. The galaxy appears to be relatively undisturbed, showing no obvious signs of recent major merger activity.
