The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The light is dominated by a bright, relatively featureless core. The outer regions display a gradual fading in intensity, suggesting a lack of significant spiral arm structure or distinct star-forming regions. There is a subtle elongation to the galaxy's shape, indicating a deviation from perfect circularity. Overall, the galaxy appears to be a quiescent system with little evidence of ongoing star formation or major disturbances.
