The galaxy presents an overall elliptical morphology, appearing largely smooth with a high degree of central concentration. It exhibits a moderate axis ratio, appearing somewhat elongated but not extremely so. Color gradients are subtle, with a central region appearing more yellow/orange, suggesting an older stellar population, which transitions to slightly bluer hues in the outer regions, implying the presence of some younger stars. There are no prominent spiral arm structures, dust lanes, or indications of ongoing major mergers visible in the image. There may be faint hints of minor disturbances in the surrounding halo. Overall, the galaxy appears to be a relatively undisturbed, evolved system with moderate star formation activity.
