The galaxy presents as a singular, relatively smooth and concentrated entity. The morphology appears largely spheroidal, exhibiting a high degree of central concentration with a gradual decrease in luminosity towards the outer regions. The overall color profile suggests a predominantly older stellar population, displaying a yellow-red hue. No prominent spiral arm structures or significant dust lanes are discernible within the observed field. The lack of prominent features indicates minimal ongoing star formation. There is no evidence of active galactic nuclei activity or significant tidal disturbances from this image alone.
