The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The color profile suggests a relatively old stellar population, exhibiting a yellowish-orange hue that likely indicates a dominance of evolved stars. There is no discernible disk structure or spiral arm features. The overall shape is close to round with no obvious signs of tidal disturbances or ongoing major merger activity, though there might be a very slight asymmetry in the outer regions. The light is centrally concentrated, and the outer regions fade smoothly into the background.
