The galaxy presents an overall elliptical morphology, appearing largely smooth and featureless. There is a notable concentration of luminosity towards the center, suggesting a prominent galactic bulge or core. The light distribution transitions gradually from the core outward, lacking any sharply defined spiral arm structures or distinct dust lanes. The galaxy exhibits a subtle blue hue, most pronounced in the central region, potentially indicating recent or ongoing star formation, although at a relatively low rate. There are no obvious signs of tidal disturbances or interactions with other galaxies, suggesting that it is currently isolated or has undergone a period of relative quiescence in terms of mergers. The overall appearance suggests a galaxy that is either an elliptical galaxy or a lenticular galaxy viewed close to face-on.
