The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is somewhat elliptical, exhibiting a higher concentration of light towards its core. The galaxy displays a color gradient, transitioning from a yellowish-white hue in the central regions to a slightly bluer color in the outer regions. There is a hint of subtle structure in the disk, although it is not well-defined and appears relatively undisturbed. There does not appear to be a significant ongoing merger event occurring. The presence of bluer colors in the outer regions suggests some level of ongoing or recent star formation. Overall, the morphology indicates that the galaxy is an intermediate stage between an elliptical and a spiral galaxy.
