The galaxy presents an elliptical morphology, appearing largely smooth in texture. The light distribution suggests a high degree of central concentration with the brightest region located at the center of the object, which fades gradually toward the periphery. The galaxy exhibits a yellow-white hue at its core, which is indicative of an older stellar population. There is evidence of an extended, less luminous halo, with hints of subtle structures or irregularities that are not readily classified, though their appearance is faint. There is a minor disturbance detectable, yet no major distortion of its form. This is an isolated galaxy. 
