The galaxy presents as a single, centrally concentrated object with a smooth, elliptical morphology. It is primarily yellowish-orange, suggestive of an older stellar population. The galaxy exhibits a high degree of central concentration, with a gradual decrease in luminosity outward from the core. The overall shape is somewhat elongated but not highly distorted. There is potentially a faint secondary object in the lower section of the image, in proximity to the primary galaxy. This could indicate a minor interaction or a companion object, but this should be verified with further observation. 
