The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright core, surrounded by a less luminous, more diffuse halo. The color profile suggests a generally evolved stellar population, with a yellowish hue dominating the overall appearance. There is no readily apparent spiral structure or dust lane obscuration. There is no visual evidence of any ongoing major merger activity, though the possibility of minor disturbances or past interactions cannot be ruled out based on this image alone. The galaxy appears generally round in shape.
