The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated luminosity profile, with brightness decreasing gradually from the core outwards. There is a subtle color gradient observed. The central region presents with a warmer, yellow-red hue, transitioning to a cooler, bluish color in the outer regions. The overall shape is largely spheroidal, although a minor deviation from perfect circularity cannot be ruled out. No apparent spiral arm structures or significant dust lanes are detected within the visible portion of the galaxy. There is no visually obvious evidence of active galactic nucleus activity, major mergers, or strong tidal disturbances. Faint features hint at possible minor interactions, but these do not dominate the galaxy's overall appearance.
