The galaxy presents as a face-on spiral with relatively tightly wound arms. There appears to be a moderate-sized bulge at the galactic center, exhibiting a gradual transition in luminosity from the core to the disk. The spiral arms are prominent and demonstrate a multi-armed structure, with several arms originating from the central region. These arms show evidence of active star formation, indicated by the presence of numerous blue knots along their length, indicative of regions with younger, hotter stars. There may be a weak bar structure spanning a portion of the central region of the galaxy. Overall, the galaxy displays characteristics of a relatively undisturbed, well-defined spiral morphology.
