The galaxy presents as a face-on or slightly tilted spiral galaxy. There's a noticeable, moderately sized central bulge, appearing yellowish and brighter compared to the outer regions, which suggests an older stellar population is located there. Faint spiral arm structures are visible, though somewhat diffuse and not sharply defined. The arms show a patchy distribution of blue light, potentially indicative of ongoing star formation. The overall disk color is blueish, a sign that there is a younger stellar population and active star formation. The galaxy doesn't show any strong signs of a major ongoing merger, however, there are some minor disturbances and faint tidal features that hint at possible past interaction. There is no obvious strong bar structure.
