The galaxy presents a smooth, elliptical morphology. The light distribution appears centrally concentrated, transitioning outward to a more diffuse halo. There is a slight elongation to the galaxy's shape, suggesting it is not perfectly spherical. Color gradients are subtle, with a yellowish central region potentially indicative of an older stellar population, fading out to a bluer edge. No distinct spiral arm structures or prominent dust lanes are discernible in this image. The galaxy exhibits a relatively compact structure. There is a suggestion of minor asymmetry in the outer regions, however it is not pronounced. The galaxy is likely quite massive, with a moderate rate of star formation.
