The galaxy appears as a centrally concentrated object with a somewhat smooth overall morphology. It presents an elliptical-like shape, though not perfectly round. The central region is characterized by a bright, yellowish-white core, likely indicative of a high concentration of older stellar populations. Moving outwards from the core, the galaxy exhibits a gradual decrease in brightness. There's a hint of a faint, bluer outer disk component, suggesting the presence of some younger stars or ongoing star formation, although limited. No prominent spiral arms or other distinct features are discernible. The galaxy shows no obvious signs of major mergers or significant tidal disturbances, though a minor disturbance cannot be ruled out. 
