This galaxy appears to be a spiral galaxy with a prominent disk. The arms are tightly wound around the central bulge and extend outwards, indicating a well-defined spiral structure. The bulge appears to be of moderate size, contributing significantly to the galaxy's overall luminosity.

There is evidence of a slight bar structure in the central region. The arms exhibit some clumpy regions, possibly indicating areas of active star formation. Overall, the galaxy seems to be relatively undisturbed, showing no major signs of recent mergers or interactions, though there could be minor disturbances. The galaxy is not edge-on, instead at an angle to us.
