The galaxy presents as a smooth, elliptical-like structure with a dominant central bulge. The light distribution appears concentrated towards the center, exhibiting a radial decrease in intensity. There is a subtle color gradient visible, transitioning from a yellow-ish hue in the core region to slightly redder tones in the outer halo. No distinct spiral arms or significant dust lanes are discernible, suggesting a lack of prominent ongoing star formation. The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions. The morphology points towards a population of older stars, likely dominated by late-type giants and dwarfs. The overall structure appears relatively symmetrical and well-defined, indicating a dynamically evolved system.
