The galaxy exhibits a smooth, elliptical morphology with a relatively high degree of central concentration.  The overall color appears yellowish, suggesting an older stellar population. There is no evidence of strong spiral arm structure or active star formation regions visible in this image. The galaxy appears more elongated in shape than circular, though not to a great degree. No signs of tidal disturbances or ongoing mergers are detected within the image, although subtle disturbances could be obscured by the limitations of image resolution. It is a relatively large galaxy, with a high mass estimate.
