The galaxy presents as a spiral type, exhibiting a noticeable disk structure. While not perfectly edge-on, the disk appears tilted relative to our line of sight. Two well-defined spiral arms are visibly emanating from the central bulge. The winding of these spiral arms appears to be of intermediate tightness. 

A central bulge is clearly present, estimated to be moderate in size. There is some indication of a bar structure within the central region, though it does not appear to be a prominent feature.

There is evidence of ongoing star formation activity throughout the disk, indicated by the bluer color within the spiral arms. The galaxy doesn't appear to be undergoing any major merging events, although there are some minor disturbances possibly suggesting past interactions. 
