The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a central bulge that appears bright and concentrated, with a gradual decrease in luminosity towards the outer regions. The shape is somewhat elongated, displaying a moderate degree of ellipticity. There is no strong evidence of prominent spiral arms or a well-defined disk structure. Faint irregular features are possibly indicative of minor disturbances within the galaxy's structure, but no significant ongoing merger event is apparent. The galaxy color suggests an older stellar population, dominated by redder stars, though some bluer regions are visible, potentially indicating areas of recent, though limited, star formation.
