The galaxy presents as a somewhat rounded, singular object with a relatively smooth appearance. The overall color profile suggests a slightly more aged stellar population. A slight extension exists, creating a deviation from a perfectly circular shape. There is a hint of a possible secondary nucleus or brighter region offset from the primary center. Based on its appearance and estimated distance from the redshift, it is likely a substantial galaxy with ongoing, but not exceptionally vigorous, star formation. It doesn't appear to be strongly interacting or undergoing any major mergers, exhibiting only a minor asymmetry.
