The galaxy appears to be a spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. The spiral arms are well-defined, though somewhat patchy, and display a bluer color, indicating the presence of younger stars and ongoing star formation. The spiral arms appear to exhibit signs of grand design structure with distinct formations branching from the central nucleus. Some dust lanes are subtly visible within the spiral arms, particularly on one side of the nucleus. There are also a few potential HII regions in the arms, appearing as bright, slightly irregular knots. The overall structure does not suggest a major merger, but possibly a minor interaction or disturbance. The system is moderately inclined relative to the line of sight.
