The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be mostly featureless, lacking prominent spiral arms or significant dust lanes. The central region exhibits a brighter, concentrated luminosity, suggestive of a dense core. The galaxy displays a subtle color gradient, shifting from a blueish hue in the central region to redder tones in the outer areas, implying a differential distribution of stellar populations and possibly ongoing, though subdued, star formation. The overall shape is slightly elongated, with an intermediate axis ratio indicating a moderate degree of ellipticity rather than being perfectly spherical. There are no immediately obvious signs of major mergers or significant tidal disturbances in this image. There are very faint indications of minor disturbances in the outer regions, warranting a closer look.
