The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile. The central region is visibly brighter, transitioning to a gradual decrease in luminosity towards the outer edges. A subtle color gradient is detected, the core region appears blue, indicative of younger stellar populations or potentially active galactic nuclei (AGN) activity, while the halo exhibits a slightly redder hue, potentially indicative of older stars or dust. There is a hint of a disk. The overall light distribution suggests a spheroidal structure. There is the possibility of a minor merger or tidal interaction.
