The galaxy presents a primarily smooth morphology, exhibiting a largely spheroidal shape. The central region displays a bright, concentrated luminosity, suggestive of a prominent galactic nucleus or bulge. A subtle color gradient is observed, with a shift toward redder hues in the core, which could potentially be due to an older stellar population or dust obscuration. The outer regions display a gradual decrease in luminosity, exhibiting a somewhat diffuse halo with a hint of blue, indicative of a younger stellar population. There is subtle evidence of mild disturbances in the morphology. These features do not appear to represent a major interaction.
