The galaxy presents a largely smooth and elliptical morphology. The overall color appears to be dominated by a yellowish-white hue, suggesting a population of older stars with relatively low ongoing star formation. The galaxy exhibits a high degree of central concentration, with light intensity decreasing gradually from the core. The isophotes appear mostly regular, indicating a relaxed dynamical state with no obvious signs of recent major mergers or tidal disturbances. There is a subtle color gradient, with the core appearing slightly redder than the outer regions. The shape is close to round, with only a slight deviation from circularity. There are no clearly defined spiral arms or prominent dust lanes visible within the galaxy's structure. Overall, the galaxy appears to be a massive, evolved system, likely hosting a supermassive black hole at its center.