The galaxy presents as a single, luminous object with a smooth, elliptical morphology. There is a centrally concentrated, bright core that exhibits a yellowish-white hue. The outer regions fade in intensity, transitioning to a bluer color. The smooth appearance suggests that this system has largely completed its merger history and is now dominated by an older stellar population in an established spheroid. There is little evidence of spiral arm structure or significant dust lanes. The overall structure suggests a relatively evolved system, potentially a massive elliptical galaxy with a substantial stellar mass. The slight blue tinge in the outer edges may indicate a small population of younger stars in these regions, hinting at continuing, low-level star formation. No obvious signs of major tidal disturbances or ongoing merger activity are present.
