The galaxy appears as a singular, concentrated body of light, generally elliptical in shape, with a smooth, featureless texture. Its color is predominantly a yellowish-orange hue, indicative of an older stellar population. There is a distinct central bulge, which is the brightest region of the galaxy. The light intensity decreases steadily from the center outwards. The galaxy's overall structure suggests it is not actively undergoing any major merging events or significant disturbances. No spiral arms or dust lanes are clearly discernible. It presents as a relatively evolved galaxy with a stable morphology.
