The galaxy presents a generally smooth, elliptical morphology. It appears to be a relatively round object, although there is a slight elongation along one axis. The light distribution is concentrated towards the center, suggesting a prominent bulge. There's a distinct color gradient, transitioning from a yellowish core to a bluer outer halo. The overall structure does not show any signs of significant disturbances or ongoing major merging events. Faint and diffuse features may be present in the outer regions, but more detailed imaging would be required to ascertain if those are indeed separate objects in the process of a merger. The smoothness and color profile hint at a relatively evolved system, dominated by older stellar populations, but it also appears to have ongoing star formation based on the bluer colors in the outer region.
