The galaxy presents a smooth, elliptical morphology. Its light profile appears relatively uniform, with a high degree of central concentration that decreases gradually toward the outer edges. The color gradient suggests a stellar population dominated by older stars. The galaxy is largely featureless, with no prominent spiral arms, dust lanes, or other indications of recent or ongoing major merger events. There are only slight indications of a blueish halo. The overall symmetry and shape suggest it is not undergoing major gravitational interactions, but slight disturbances may be present.
