The galaxy presents as a spiral galaxy with a relatively prominent disk structure. The spiral arms are well-defined and exhibit a moderate winding, not tightly wound nor completely loose. Two dominant spiral arms are discernable. The bulge appears to be small to moderate in size relative to the overall galactic structure. There's no clear evidence of a strong bar feature, though a weaker bar presence can not be ruled out. There is no clear evidence of any major merger events or significant tidal disturbances. The overall color suggests ongoing star formation within the disk and spiral arms.
