The galaxy presents as a spiral, viewed at a slight angle from face-on. It exhibits two prominent spiral arms emanating from a bright central bulge or core. The arms appear relatively tightly wound near the core, becoming less defined as they extend outwards. The bluer color in the arms suggests the presence of active star formation. The galaxy displays an overall circular shape, but subtle irregularities in the arm structure hint at possible gravitational interactions or internal disturbances. There is a bar-like structure connecting to the nucleus, further suggesting that the galaxy is in a state of change.
