The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high surface brightness, with a gradual decrease in luminosity towards the outer edges. There appears to be a subtle color gradient, with the core showing a slightly bluer hue and the outer regions appearing redder. No distinct spiral arms or bar structures are evident. The overall shape is generally round, showing little deviation from circular symmetry. There is no evidence of major disturbances, tidal tails, or other signs of recent merger activity, suggesting a relatively quiescent state. The galaxy appears as an isolated system.
