The galaxy presents a largely smooth, elliptical morphology. It appears almost spheroidal, with a high degree of central concentration of light. The galaxy exhibits a color gradient, appearing more yellow-orange toward the core and transitioning to a bluer hue in the outer regions. The apparent angular size of the galaxy is relatively small, suggesting a considerable distance. There is a subtle hint of distortion in the galaxy's shape, possibly due to a minor gravitational interaction or ongoing merger event, though this is difficult to ascertain with certainty based solely on the available imagery. The galaxy appears as an isolated system with no clear signs of major disturbances. 
