The galaxy presents as a spiral type, with a generally face-on orientation relative to our line of sight. A prominent bar-like structure is observed through the central region. Two well-defined spiral arms originate from the ends of the bar, winding outwards in a grand design. Patches of blue light are scattered throughout these arms, suggestive of active star formation regions. Dust lanes are visible, tracing the inner edges of the spiral arms. The central bulge appears relatively small and unobtrusive. The overall structure exhibits some disturbances, possibly indicating a past or ongoing minor interaction with another galaxy. The galaxy's disk shows a clear rotational pattern.
