The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The light is concentrated towards the center, indicating a high degree of central mass concentration. The galaxy exhibits a color gradient, with a yellowish-white hue towards the core transitioning to a bluer periphery, suggestive of ongoing star formation at a relatively low rate in the outer regions. The galaxy’s shape is more elongated than circular, implying a degree of rotational support, but appears to be closer to a flattened sphere. There is no evidence of major tidal disturbances or mergers, implying it has had a relatively calm recent history.
