The galaxy presents as an elliptical morphology, exhibiting a smooth and concentrated light profile. The central region displays a yellowish-white hue, suggesting an older stellar population. The galaxy appears quite round in shape, showing minimal deviation from circular symmetry. There are no apparent signs of spiral arms or a prominent disk structure. The overall appearance indicates a relatively undisturbed system, with no obvious tidal features or indications of recent merger activity. The observed color suggests moderate star formation, with the presence of both older and some younger stars.
