The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The core region exhibits a high degree of luminosity, suggesting a concentration of older stars. The galaxy displays a slightly elongated shape, though it largely approximates a spherical form. There is no apparent indication of ongoing major merger activity or significant tidal disturbances. The overall color profile suggests a population dominated by relatively old stars, with a low rate of star formation.
