The galaxy presents as a spiral type, viewed at an oblique angle, but not quite edge-on. There are signs of loosely wound spiral arms emanating from a central bulge. The bulge appears to be a moderate size relative to the overall disk. Patches of star formation are suspected within the arms based on color variations. A bar-like structure is potentially present, but difficult to definitively confirm given the image's resolution. The overall morphology suggests a galaxy undergoing active star formation, though perhaps at a moderate rate. There is a suggestion of minor disturbances in the galaxy's structure, possibly indicating a past or ongoing interaction with a smaller companion galaxy.
