This galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core with a yellowish-orange hue, suggesting an older stellar population. Moving outwards from the core, the color gradually shifts towards a redder tone, still indicative of aging stars. The overall shape is close to circular, showing only a slight deviation towards an elongated form. The outer edges of the galaxy appear somewhat diffuse, without any clearly defined spiral arms or distinct disk structures. There is a faint hint of possible minor disturbance on one side, but no prominent signs of ongoing major merger activity are observed. Overall, this appears to be a relatively undisturbed elliptical galaxy.
