This galaxy appears as a compact, elliptical system. Its light profile seems smooth, exhibiting no distinct spiral arm structures or a prominent central bar. The dominant color is a yellowish-red hue, suggesting a stellar population that is primarily older, with lower levels of on-going star formation. There are no obvious signs of recent or ongoing mergers, although the light distribution isn't perfectly regular, with some subtle irregularities suggesting minor disturbances may have occurred in the past. The round morphology indicates a system that is likely supported by mostly random stellar motions, typical of elliptical galaxies at this distance.
