The galaxy presents a slightly elongated, elliptical morphology. Its central region exhibits a concentration of light with a yellowish-orange hue, suggesting an older stellar population. Surrounding the core, there's a more diffuse, bluish halo indicative of a younger population. The smooth light distribution suggests it is a relatively mature system with ongoing, but not particularly vigorous, star formation. There are subtle signs of minor disturbances in the outer regions, potentially indicating past or ongoing interactions with smaller satellite galaxies. The galaxy's overall appearance is generally smooth and well-defined, though not perfectly symmetrical. 
