The galaxy presents a generally smooth and elliptical morphology. Its light is concentrated towards the center, indicating a prominent nucleus. The color is yellowish-white, suggesting a dominant population of older stars. There is a lack of defined spiral arms or significant dust lanes, which would indicate features. The overall round shape suggests a system without a strong rotational component. There's no obvious evidence of recent or ongoing major merger activity. Some minor distortions are possible. The galaxy seems relatively isolated and well-defined. Based on the observed characteristics, this appears to be a fairly massive elliptical galaxy.