This galaxy appears to be a spiral galaxy at an estimated distance, as indicated by its redshift. Its apparent angular size suggests it's a relatively compact galaxy. The central bulge is moderately prominent, exhibiting a smooth, slightly elongated structure. The spiral arms appear somewhat diffuse and not tightly wound, showing a flocculent structure, with some patches of bluer regions possibly indicating areas of active star formation. There is a noticeable gradient in color from the center outwards, with the core appearing yellower, which could indicate an older stellar population, to bluer arms, hinting at younger, hotter stars. There are possible signs of tidal interactions.
