The galaxy presents as a centrally concentrated, elliptical-like structure. Its morphology is dominated by a smooth, relatively featureless light distribution. The core region exhibits a bright, yellowish-orange hue, which gradually fades into a more diffuse halo with a slightly greener tint towards the edges. There is no discernible spiral arm structure or dust lane visible. The overall shape suggests a relatively evolved system with minimal ongoing star formation. There might be minor disturbances but nothing conclusive. The galaxy does not appear to be undergoing a major merger.
