The galaxy presents as a relatively smooth, elliptical structure. It exhibits a bright, concentrated central region, likely indicative of a substantial galactic nucleus. The overall shape appears largely spherical, showing minimal deviation from a circular form. A subtle color gradient is observed, with the core displaying a more yellowish hue, possibly associated with an older stellar population, transitioning to a slightly redder tinge in the outer regions. There are no prominent spiral arms, bars, or other distinct features discernible, suggesting a lack of significant ongoing star formation in a well-defined disk structure. There are no apparent signs of major galactic mergers or tidal disturbances in this image, which further supports its classification as an elliptical galaxy exhibiting a high degree of regularity.
