The galaxy presents as a spiral type, with a relatively small, moderately bright central bulge. The disk is viewed nearly face-on, exhibiting well-defined spiral arm structures. These arms appear tightly wound, emanating from the central bulge and extending outwards. The arms show a clumpy texture, suggestive of active star formation regions. The overall color of the spiral arms is bluer than that of the central bulge, which has a yellower hue, indicative of an older stellar population. There is no apparent bar structure bisecting the central region. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions with other galaxies.
