The galaxy exhibits a generally smooth morphology, appearing largely elliptical in shape. A discernible central bulge is present, with a yellow-orange hue, suggesting a population of older stars. The overall color gradient indicates a higher concentration of older stellar populations in the core, gradually transitioning to a slightly bluer halo. Though largely smooth, there is a subtle indication of a faint, extended disk component, slightly elongated. There is no obvious indication of active star formation within this object, nor of any major ongoing mergers. The galaxy appears relatively undisturbed.
