The galaxy presents as a spiral type with a prominent disk structure. Evident spiral arms emanate from a central region. The arms appear somewhat tightly wound, although detailed substructure within the arms is not clearly resolved. The bulge component is moderate in size. The galaxy exhibits a noticeable inclination relative to our line of sight, suggesting we are not viewing it perfectly face-on. There is a hint of asymmetry and disturbance within the morphology, possibly indicating ongoing or past interaction or minor merger. Light distribution is concentrated at the center, where light and color are most intense.
