The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a color gradient, appearing brighter and more yellow-white in its central regions, suggesting a concentration of older stellar populations. There is a gradual decrease in surface brightness moving outward from the core. The overall shape is close to but not entirely round; it seems somewhere between round and elongated. There is no visible spiral structure or prominent dust lanes, and based on its appearance, it is likely not undergoing any major mergers or experiencing significant tidal disturbances.
