The galaxy presents as a centrally concentrated, relatively smooth, and somewhat elongated structure. Its color profile indicates a yellowish-white hue, suggesting a population of older stars with relatively low ongoing star formation. The overall shape is elliptical, with a high degree of roundness. There is no obvious indication of spiral arms or a significant disk component. No tidal features or major disturbances are visible, and the galaxy appears to be relatively isolated and unperturbed. It could possibly be undergoing a minor merger. 
