This galaxy presents a somewhat disturbed morphology. There is a suggestion of spiral arm structure, but it is not well-defined. A central bulge is present, although it appears relatively small in proportion to the overall galactic disk. The color distribution indicates ongoing star formation, concentrated in the regions suggesting spiral arms. Evidence of a possible interaction or minor merger event appears present, deforming the spiral structure. There is a noticeable lack of a dominant central component, suggesting a relatively late-type spiral galaxy. Some regions of the galaxy exhibit bluer hues, indicative of younger stellar populations, while other regions display yellower, possibly older, stellar populations. There is no obvious strong central bar structure within the galaxy.
