The galaxy presents a generally smooth, elliptical morphology. It exhibits a central bulge region that appears more concentrated and has a relatively smooth texture. The overall color profile suggests an older stellar population, with a subtle color gradient from the core outwards. There is little to no indication of prominent spiral arms or dust lanes within the galaxy. The galaxy exhibits no apparent signs of major mergers or significant tidal disturbances. It appears to be relatively undisturbed and well-defined.
