The galaxy presents as a face-on or slightly inclined spiral structure, with a dominant disk component. The spiral arms are somewhat flocculent and exhibit a patchy distribution of star formation, as evidenced by the presence of blue-tinged regions indicating areas of active star birth. There is no distinct, bright bulge component at the center, suggesting either a small or non-existent central bulge. Overall the galaxy has a complex structure, possibly indicating a merging event or gravitational interaction with another galaxy. The galaxy exhibits evidence of recent or ongoing minor merger activity.
