The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical with a high degree of roundness. A discernible core exhibits a yellowish-white hue, suggesting an older stellar population. There's a faint gradient toward the outer regions, with a subtle color shift towards redder tones, further reinforcing the impression of evolved stars. No spiral arm structures or significant dust lanes are evident. There are no apparent signs of recent or ongoing major merger activity, though some very minor internal disturbances cannot be ruled out. The overall appearance is consistent with an early-type galaxy at intermediate redshift.
