The galaxy presents as a generally smooth, elliptical morphology, with a high degree of central concentration. The light profile appears relatively symmetrical, exhibiting a gradual decrease in luminosity moving outward from the core. There is a slight elongation visible, suggesting a deviation from perfect sphericity. The core region shows a yellowish color, potentially indicating an older stellar population. The outer regions display a faint bluish tint, hinting at a small amount of recent star formation activity, though it's not particularly prominent. There is no clear evidence of spiral arms or a well-defined disk structure. No signs of tidal disturbances or ongoing major mergers are apparent, though there may be minor asymmetries.
