This galaxy appears to be a relatively smooth, elliptical-type system at a moderate redshift. Its central region exhibits a strong concentration of light, appearing a yellow-white hue, suggesting a population of older stars. The galaxy is generally round in appearance. There is no indication of significant disk structure, spiral arms, or ongoing major mergers. Minor asymmetry may be present, but this could also be image noise. The outer regions of the galaxy show a gradual decrease in luminosity. The colors present seem to indicate low levels of star formation.
