The galaxy presents as a relatively smooth, centralized distribution of light. It exhibits an elliptical morphology, appearing largely spheroidal in shape, with a high degree of roundness. No distinct spiral arm structures or prominent disk features are discernible. The galaxy displays a slight color gradient from the center outwards, with a bluer core potentially indicating regions of recent or ongoing star formation, transitioning to a slightly redder halo suggestive of an older stellar population. There is no apparent evidence of significant morphological disturbance or ongoing merger activity.
