The object presents as a relatively smooth, elliptical galaxy. Its morphology is characterized by a centrally concentrated luminosity profile, with a gradual decrease in brightness radiating outward from a bright core. The galaxy exhibits a distinct reddish-yellow hue, suggesting a predominantly older stellar population and a lower rate of on-going star formation. There is no apparent evidence of spiral arms, significant dust lanes, or recent merger activity within the resolution limits of this image. The shape appears close to circular.
