The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated luminosity profile, with the light generally concentrated in the center of the object. The shape is not perfectly spherical, but rather somewhat elongated. There is some evidence of a disk, though only a small fraction of the galaxy shows that.

There is little sign of significant star formation, and given its red color, the galaxy is composed largely of older stellar populations. The galaxy does not exhibit signs of ongoing or recent merger activity.
