The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a spheroidal morphology, lacking any obvious spiral arm structures or a prominent disk. The central region is characterized by a bright, yellowish-orange hue, suggesting an older stellar population or significant dust obscuration. The outer regions display a gradual decrease in luminosity, fading into a bluish-green tinge. This color gradient could indicate the presence of younger stars and ongoing star formation in the galaxy's outer reaches, but the overall smoothness suggests this may not be a strong presence. No signs of significant tidal disturbances, major mergers, or close companion galaxies are discernible. Overall, the galaxy appears to be a relatively isolated, well-defined system.
