The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The central region exhibits a distinct yellowish-orange hue, suggesting a population of older stars. The galaxy appears largely elliptical, trending towards a rounded shape. Fainter, bluer light is observed in the surrounding regions, hinting at potential star formation activity, although minimal overall. No obvious spiral arm structure or bar features are discernible in the image. There are no immediately apparent signs of major tidal disturbances or ongoing mergers, although subtle asymmetries may indicate minor past interactions. The overall appearance indicates a mature galaxy with a significant spheroidal component.
