The galaxy presents an overall elliptical morphology, exhibiting a smooth, concentrated light distribution. The core is bright and appears slightly elongated. The light profile of the galaxy appears to decrease smoothly with increasing radius. The galaxy appears to have a central bulge and a hint of a disk. There is no apparent active galactic nuclei. No significant dust lanes or spiral arm structures are observed. There does not appear to be any ongoing merging activity or signs of tidal disturbances.
