The galaxy presents as a relatively smooth, elliptical-like structure. It is highly concentrated towards the center. The light distribution suggests a centrally dominant stellar population. There is little evidence of spiral arms or a distinct disk component. Color gradients are subtle, with a slight blue hue indicating a very small amount of on-going star formation. No major mergers or significant tidal disturbances are visibly evident. The morphology appears undisturbed, suggesting a settled or quiescent state.
