The galaxy presents an elliptical morphology. Its light profile is centrally concentrated with a smooth, diffuse halo fading into the background. The core exhibits a yellowish hue, suggesting an older stellar population. The overall shape deviates slightly from perfectly circular, displaying a moderate elongation along one axis, perhaps indicating it is more disk-like than purely elliptical. There are no visible signs of spiral arms, active star formation regions, or major disturbances indicative of recent merger events. Faint indications of minor irregularities are suggested, though they are not prominent features. The color gradient from the core to the outer regions appears minimal.
