The galaxy presents as a largely smooth, elliptical structure. It exhibits a high degree of central concentration, with the luminosity peaking sharply towards the galactic core. The overall shape appears close to circular. There is little to no indication of distinct spiral arms or a pronounced disk component. The galaxy appears to be relatively isolated, showing no signs of ongoing major mergers or tidal disturbances, although a very slight asymmetry or minor irregularity cannot be completely ruled out. The color profile suggests a redder overall population, consistent with an older stellar population and subdued star formation activity. Based on its characteristics, a classification as an elliptical galaxy is likely.
