The galaxy presents as a relatively smooth, lenticular-like structure with an apparent high degree of central concentration. The morphology appears to be largely spheroidal, with some evidence of a faint disk component. The galaxy exhibits a subtle color gradient, with a bluer hue around the main body of the galaxy and possibly the beginnings of faint arms near the edge of the spheroid. The overall color suggests a population of older stars and a very low rate of current star formation. There is a very slight distortion in its shape, possibly from an ongoing or past minor interaction. There is no obvious active galactic nucleus. The estimated size is approximately 2.3 kpc in radius.
