The galaxy presents a largely smooth, elliptical morphology with high degree of central concentration. It appears nearly circular, with a subtle deviation from perfect roundness. The light profile suggests a single component system, lacking evidence of significant spiral arm structure or distinct disk features. The color is dominated by a yellowish hue, indicating a population of older stars with relatively little ongoing star formation. There is no visible evidence of tidal disturbances or active galactic nuclei activity in the image. The galaxy does not appear to be actively merging or interacting with any other galaxy based on current data.
