The galaxy presents as a spiral type, exhibiting well-defined spiral arms emanating from a central bulge. The spiral arms appear flocculent, displaying clumpy regions of star formation with a blueish hue indicative of young, hot stars. The bulge appears yellowish, suggesting an older stellar population. There is an indication of a bar structure. The galaxy appears slightly inclined relative to our line of sight. There seems to be no major ongoing merging activity, but minor disturbances can't be ruled out.
