The galaxy presents as a smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity moving outward. The color profile suggests an older stellar population, dominated by redder hues, particularly towards the core. There is a hint of bluer light on the edges of the disk, this could be caused by a small amount of star formation occurring on the edges. The galaxy lacks any prominent spiral arms or significant dust lanes, lending to its smooth overall appearance. The morphology appears generally undisturbed, without obvious signs of ongoing or recent major merger events.
