The galaxy is a centrally concentrated system exhibiting a smooth morphology. It appears elliptical in shape, with a high degree of central concentration in luminosity. There is a distinct color gradient from the central region outwards, with the nucleus displaying a more yellowish-white hue, transitioning to a reddish color in the outer regions. There is no evidence of spiral arms or significant dust lanes. The object is not perfectly round but also is not elongated, it appears to fall in between the two. The overall appearance suggests it is not currently undergoing any major merging events, and if it is merging, it is likely due to a minor disturbance. The data suggests this is a massive galaxy with a relatively low star formation rate.
