The galaxy presents as a roughly elliptical structure, exhibiting a high degree of central concentration. The core region displays a significantly brighter luminosity, transitioning smoothly outwards to a fainter halo. There appears to be little evidence of a distinct disk structure, with a generally smooth overall appearance. Color gradients are subtle, with a redder core gradually shifting toward bluer hues in the outer regions. There is no obvious presence of spiral arms or significant dust lanes. No strong signs of ongoing major merger events can be observed. The galaxy has a substantial mass. The rate of new star formation is very low. 
