The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated light distribution. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears to be fairly rounded, with a slight elongation. The color of the galaxy exhibits a yellowish-red hue. The morphology suggests that the galaxy is relatively evolved and likely hosts an older stellar population. There is no obvious signs of tidal disturbances or ongoing mergers, although there are a few galaxies located very close to it in the image.
