The galaxy presents a generally smooth and elliptical morphology. A bright, concentrated central bulge dominates the structure, appearing nearly spherical. Surrounding the bulge is a fainter, more diffuse halo or disk component. The disk appears only subtly, with a slight elongation on one side of the bulge. There is a hint of spiral structure. This is supported by color gradients; the central bulge exhibits a yellow-white hue, suggesting an older stellar population, while the subtle disk shows a bluer tint. It suggests ongoing or recent star formation. There is a slight chance that it is undergoing minor disturbances. Overall, the galaxy gives an impression of a relatively evolved system with a significant spheroidal component and a lower star formation rate.
