The galaxy presents as a spiral type, observed at a redshift indicating a considerable distance. Its central region exhibits a pronounced bulge component, a concentrated area of older stellar populations giving off yellowish light. Emerging from the bulge are faint spiral arms, displaying subtle blue hues indicative of ongoing star formation. These arms appear somewhat flocculent in nature, lacking a grand, well-defined design. There is suggestion of a bar-like structure that is oriented through the center of the galaxy. The galaxy's morphological classification leans towards a late-type spiral galaxy. Based on the observed features, it seems to be in a relatively unperturbed state.
