The galaxy presents as a somewhat elliptical, relatively smooth object. It has a noticeable central bulge that appears brighter and more concentrated than the outer regions. The color gradient suggests a relatively older stellar population, with a yellowish-orange hue dominating the core. The outer regions appear slightly bluer, suggesting the presence of younger stars, though not prominently. The galaxy exhibits a moderate degree of flattening. No distinct spiral arm structure or significant dust lanes are discernible in this image. There is no clear sign of ongoing major merger activity, although some minor tidal disturbance cannot be ruled out based on the image alone.