The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge region that is bright, transitioning to a dimmer, more diffuse halo extending outwards. Color gradients suggest a variation in stellar populations; the core appears more yellow to white in color, while the outer regions display a reddish hue. There are no prominent spiral arm features or evidence of significant dust lanes visible in this image. There is a slight irregularity to its overall elliptical shape, though no major distortions are apparent, suggesting no ongoing or recent major merger activity, though minor disturbances cannot be ruled out. Based on the overall color and morphology, it likely represents a mature galaxy with a relatively low rate of current star formation.
