The galaxy presents as a centrally concentrated, elliptical-like object, with a smooth light distribution indicative of an early-type system. A noticeable radial color gradient is observed, transitioning from a redder core to bluer outer regions. The overall morphology suggests a system that is relatively undisturbed, without apparent signs of major mergers or significant tidal interactions. There are no prominent spiral arms or distinct features associated with active star formation that are visible in the image. Some minor irregularities in the outer halo are visible, which may indicate minor tidal interactions or low-level star formation.
