The galaxy appears as an elliptical morphology, with a smooth, centrally concentrated light profile. It exhibits a moderate ellipticity, appearing somewhat flattened. The core region displays a yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, a subtle color gradient is observed with a transition towards blueish tones in the outer regions of the galaxy, which could suggest a presence of younger, hotter stars. No distinct spiral arms or prominent dust lanes are apparent. The overall structure indicates a relatively relaxed system, lacking signs of major recent mergers or strong tidal interactions. It shows no signs of any significant disturbances. The size indicates that it is likely to be a dwarf galaxy, possibly with ongoing, but limited, star formation.
