The galaxy presents as a face-on spiral galaxy, exhibiting a well-defined disk structure. The spiral arms are tightly wound and appear somewhat fragmented, indicating a complex star formation history and/or gravitational interactions. The central bulge is moderately sized and possesses a yellowish hue, suggesting an older stellar population. The disk shows a bluer color, particularly within the spiral arms, likely indicative of ongoing star formation and the presence of younger, hotter stars. A bar structure appears to be present, though moderately weak, extending across the central region of the galaxy. There appears to be no major merger occuring, but there is a minor disturbance present in the shape of the galaxy.
