The galaxy appears as a single, relatively smooth concentration of light. It presents an overall elliptical morphology, with a high degree of radial symmetry. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to more reddish hues in its outer regions. There is little evidence of spiral arm structures, bars, or significant dust lanes. The central region is the brightest and most well-defined. The galaxy does not display obvious signs of recent or ongoing major mergers or tidal disturbances. However, there might be a very slight asymmetry or minor distortion in its overall shape, suggesting possible past interactions. The redder color in the outer regions indicates a population of older stars, while the yellowish-white core suggests the presence of some younger stars.
