The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The color profile indicates a predominantly older stellar population, with a yellow-orange hue suggesting a lack of significant ongoing star formation. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears mostly undisturbed, without noticeable tidal features or signs of a major merger event. Overall, the galaxy exhibits characteristics consistent with an evolved elliptical galaxy.