The galaxy appears to be a spiral galaxy, observed at an oblique angle, with a clear disk-like structure. The galaxy exhibits a bright, concentrated central bulge that appears slightly elongated. Faint spiral arms extend outward from the central region, displaying a relatively tight winding. The arms show evidence of active star formation, indicated by patchy regions of blue light, likely associated with populations of young, hot stars. There may be an indication of a bar structure within the central region. The disk shows evidence of dust lanes throughout. Overall, the galaxy exhibits a substantial size and mass.
