The galaxy appears as a flattened elliptical or lenticular system, with a smooth, relatively featureless morphology. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. There is a faint suggestion of a disk component. The galaxy exhibits a subtle color gradient, with a bluer hue present throughout the structure. This color and its spectral properties may point to ongoing, although potentially weak, star formation within the galaxy, particularly when compared to the inferred total mass. The image shows no obvious signs of spiral arm structure or significant dust lanes. Overall, the morphology indicates a galaxy in a relatively evolved state, possibly transitioning from a spiral to an elliptical type. There is a noticeable elongation that seems to be its dominant form, rather than a fully round elliptical galaxy.
