The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. The core appears luminous and exhibits a near-spherical shape. Moving outward from the core, the galaxy's luminosity gradually decreases. There is a subtle color gradient visible, shifting from a slightly bluer hue in the central region to a redder tone towards the outer edges. This potentially indicates a more recent star formation in the galactic center. The outer regions show minimal structural features. No spiral arms, bars, or dust lanes are apparent, which supports the classification of this galaxy as an elliptical or lenticular type. No signs of tidal disturbances, close companion galaxies, or other indications of recent major merger events are obvious. The overall impression suggests a relatively quiescent, evolved system.
