The galaxy presents as a relatively smooth, elliptical form, with a high degree of central concentration. The core is luminous, exhibiting a yellowish-white hue that gradually diffuses into a surrounding, fainter halo. This halo displays a subtle reddish tint, hinting at a population of older, cooler stars. There's a lack of discernible spiral arm structure or prominent dust lanes; instead, the galaxy appears largely featureless. The light distribution suggests a smooth transition from the bright nucleus to the outer regions, indicating an absence of ongoing major merger activity, though there may be a slight asymmetry. The overall morphology points towards a galaxy that is transitioning, or has transitioned, from a period of active star formation to a more quiescent state. The lack of blue light suggests a low current star formation rate. It appears moderately massive.