The galaxy presents as a relatively smooth, elliptical morphology, with a high degree of central concentration. The color gradient suggests an older stellar population. The central region is dominated by a yellow-white hue, potentially indicative of a bulge rich in evolved stars. There is very little evidence of dust lanes or spiral arm structures in the image. The shape is close to round. There is no visual indication of any tidal features or mergers. Star formation is most likely suppressed within the galaxy.
