The galaxy presents a generally elliptical morphology, appearing predominantly smooth and concentrated towards the center. The central bulge exhibits a yellowish-white hue, suggesting a population of older, less massive stars. Moving outwards from the core, the galaxy displays a subtle color gradient, transitioning towards slightly bluer tones in the outer regions, indicating the presence of younger stellar populations and possibly ongoing star formation. There is some disturbance in the galaxy, which could be a small merger. 
