The galaxy appears to be a spiral galaxy, with a disk-like structure visible. It is not highly inclined, presenting a face-on view. The spiral arms exhibit a somewhat patchy morphology, suggesting ongoing star formation activity. There is a central bulge, but it does not dominate the overall structure. There appears to be minor asymmetry in the disk, potentially indicating a gravitational interaction or recent merger event, though no prominent tidal features are visible in this image. The galaxy's color indicates a mix of stellar populations, with some blue regions indicative of young, hot stars and more reddish areas suggesting older stellar populations. Overall, the galaxy presents a complex structure indicative of ongoing evolution and potential interactions.
