The galaxy presents as a somewhat symmetrical, elliptical shape with a relatively smooth light distribution. Its core appears concentrated with a gradual decrease in luminosity towards the outer regions, lacking distinct spiral arm structures or prominent dust lanes. The overall color is slightly yellowish-orange suggesting an older stellar population. There is no apparent signs of ongoing major mergers or tidal disturbances. The morphology suggests a classification towards the elliptical side, potentially an E type galaxy. The overall appearance indicates that the galaxy is relatively evolved, possibly with a low star formation rate.
