The galaxy presents a largely smooth, elliptical morphology. The core exhibits a high degree of central concentration, appearing bright and yellowish. A more diffuse halo extends outwards, exhibiting a gradual decrease in surface brightness with radial distance. The overall color profile suggests a dominant population of older stars with a lower rate of ongoing star formation. There are no visible spiral arms or distinct dust lanes. The overall structure appears undisturbed, lacking signs of any major recent mergers, though there is potentially some minor disturbance apparent in the halo region. The general roundness of the galaxy indicates a relatively low angular momentum.
