The galaxy presents as a spiral type, observed at an oblique angle relative to our line of sight. The central bulge appears relatively bright and somewhat diffuse, with a moderate size compared to the overall structure. Faint spiral arms are visible extending from the central region, though their definition is not sharp. There is evidence of blue coloration within the spiral arms, suggesting ongoing star formation. The overall structure is not highly symmetric and may show signs of minor disturbances. The galaxy appears somewhat elongated, with the major axis significantly longer than the minor axis. 
