The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish hue suggesting an older stellar population dominating the central region. There is a subtle color gradient from the core outward with hints of redder tones in the outer regions. The overall structure suggests a relatively relaxed system with minimal signs of recent major mergers or tidal disturbances. The size appears compact, indicating a relatively small galaxy. Based on color, the star formation rate is likely suppressed. 
