The galaxy appears to be a relatively luminous system at a moderate redshift, suggesting a significant distance. Morphologically, it presents a smooth, elliptical-like structure. The galaxy's light distribution is concentrated centrally, with a gradual falloff in brightness towards its outer regions. The overall color is slightly redder, particularly towards the center, suggestive of an older stellar population and lower levels of current star formation. There is potentially a second region that may be an artifact, but it is more likely some distortion of the galaxy image that may suggest it is a result of a minor gravitational interaction. There is no visual evidence of a strong disk component or prominent spiral arms.
