The galaxy presents an overall elliptical morphology. The central region exhibits a high degree of luminosity, appearing nearly unresolved and intensely bright. Moving outward from the core, a broader, less intense halo of light is observed, displaying a smooth and diffuse character. There is minimal visual evidence of spiral arms or distinct structural features within the halo. Subtle color variations are present, hinting at potential differences in stellar populations or dust distribution within the galaxy. The galaxy's edges gradually fade into the background, lacking sharp or clearly defined boundaries. Possible minor disturbance is inferred from its irregular shape. Overall, this galaxy appears to be an elliptical galaxy characterized by a bright core and smooth outer envelope, potentially undergoing minor gravitational interaction.
