The galaxy presents as a centrally concentrated object with a relatively smooth appearance. It exhibits a roughly circular morphology, with a gradual decrease in surface brightness moving from the core outwards. A distinct nucleus is observed, appearing bright and slightly off-white in color. The surrounding halo shows a faint bluish hue, potentially indicating the presence of younger stellar populations. The overall structure suggests that this galaxy is likely an elliptical galaxy, without prominent spiral arms or dust lanes. No obvious signs of ongoing major mergers are visible, although there's a possibility of a minor tidal disturbance hinted at by slight asymmetries in the outer regions of the halo.
