The galaxy appears to be a spiral galaxy, likely at a moderate redshift. It presents a distinct disk structure with prominent spiral arms. The arms are grand design, tightly wound, and exhibit a primarily blue coloration, indicative of ongoing star formation activity. A central bulge is present, showing a concentration of older, redder stars, however the redder color could also indicate the presence of dust. A bar feature may be present across the central region. There are signs of an ongoing merger or tidal disruption, though this is more uncertain. The overall morphology suggests a system undergoing active star formation and possible interaction with a nearby galaxy.
