The galaxy presents a generally smooth and centralized morphology. It appears elliptical or lenticular in shape, with a significantly brighter core region that exhibits a relatively blue hue. The light tapers off gradually from the center, showing no prominent spiral arms or distinct features. The overall color gradient suggests a population of older stars, but the blue core indicates the potential for ongoing star formation activity within the galaxy's central region. There is only a slight disturbance visible in the disc of the galaxy.
