The galaxy presents as a single, relatively smooth object. Its morphology is generally elliptical, with a higher concentration of light towards the center that gradually diminishes outward. The core exhibits a yellowish hue. This suggests the presence of an older stellar population. Fainter blue tones are present in the outer regions of the disk, possibly indicating regions of recent star formation. There does not appear to be any spiral structure nor evidence of active galactic nuclei. No significant tidal disturbances, merging companions, or asymmetries are discernible in the image.
