The galaxy presents as a largely elliptical or spheroidal system. It exhibits a smooth, concentrated light profile, indicating a lack of prominent spiral arms or a well-defined disk structure. The core region is bright and intensely luminous, suggesting a high density of stars or an active galactic nucleus. Surrounding the core, there is a more diffuse halo of light, fading gradually into the background sky. A slight blue tint can be detected particularly in the surrounding halo, suggesting that the outer regions may have some younger star formation. Overall, the galaxy shows no strong signs of recent major merger events or significant tidal disturbances.
