The galaxy presents as an elliptical morphology with a notably smooth profile, exhibiting minimal discernible features such as spiral arms or dust lanes. The central bulge is dominant and appears spheroidal. The radial color gradient suggests a more intense concentration of older stellar populations towards the center. The galaxy is characterized by a yellowish hue, indicating a lack of significant recent star formation, consistent with a population of primarily older, redder stars. The outer regions of the galaxy are fainter and gradually fade into the background sky, suggesting a well-established, quiescent system. No signs of tidal disturbances or ongoing mergers are visible in this image.
