The galaxy exhibits a smooth, elliptical morphology. A bright central bulge is clearly visible, gradually fading into the outer regions. The overall color profile suggests an older stellar population, with a dominance of redder hues. There is a slight elongation of the galaxy's shape, deviating from a perfect sphere. No distinct spiral arms or significant dust lanes are apparent. The galaxy appears relatively undisturbed, showing no obvious signs of recent major merger events or tidal interactions. 
