The galaxy presents a generally smooth, elliptical morphology, appearing highly centralized with a bright, concentrated core. The light distribution appears quite uniform, lacking prominent spiral arms or distinct features. The galaxy exhibits a moderate degree of roundness, deviating only slightly from a perfect circle. There is no evidence of ongoing major mergers or significant tidal disturbances in this image. The color profile suggests a population dominated by older stars, giving it a yellowish hue. This is consistent with a low star formation rate. The galaxy's overall structure indicates it is likely a massive system.
