The galaxy appears as a somewhat elliptical-shaped structure with a dominant central bulge. The light distribution is relatively smooth, suggesting an evolved stellar population. A faint disk-like component is possibly present, hinted at by a slight extension of the galaxy's light along one axis. There is a subtle hint of asymmetry. The overall color is skewed toward redder wavelengths, and the galaxy is likely at a moderate distance, indicated by the redshift and apparent size. The absence of strong blue regions suggests a relatively low ongoing star formation rate. The morphology indicates it is unlikely to be undergoing a major merger. There might be a hint of a minor disturbance, although that is not clear in the image.
