The galaxy presents a largely smooth, elliptical morphology. It exhibits a significant central bulge that appears yellowish, suggesting an older stellar population. The overall shape is somewhat elongated. There is a gradual fading of light intensity from the center outwards, with no distinct spiral arm structures visible. A subtle color gradient is observed, shifting from yellow/white in the core to a bluer hue in the outer regions. This suggests ongoing or recent star formation in the outer disk of the galaxy. There are no apparent signs of major tidal disruption or ongoing mergers. The structure is overall undisturbed.
