This galaxy appears to be a spiral, observed at an oblique angle. It exhibits a well-defined spiral structure, the arms tightly wound around a luminous central bulge. The bulge itself seems relatively small compared to the overall size of the galaxy. The spiral arms show indications of active star formation, marked by subtle variations in color, possibly caused by the presence of HII regions or young, hot stars. A faint bar structure could possibly be present at the galaxy's center, but it isn't particularly pronounced. There are no obvious signs of major interaction or merging events, although a slight asymmetry in the outer disk regions hints at a potential minor disturbance.
