The galaxy presents as a relatively smooth, centrally concentrated object. There is little indication of spiral arm structure. The galaxy exhibits a fairly circular morphology. The dominant color is a pale bluish-white, suggestive of a population of intermediate-age stars, however there is also a hint of a yellow core. The galaxy appears undisturbed, with no obvious signs of tidal tails, plumes, or strong distortions indicative of a recent major merger event. Given its distance, we can infer that this galaxy has a substantial stellar mass. However, the high rate of star formation, hints at some ongoing star-forming activity.
