The object appears to be a spiral galaxy, exhibiting a well-defined disk structure. The spiral arms are loosely wound. The galaxy's color suggests a mix of stellar populations, with a yellow-orange hue in the central bulge potentially indicating older, redder stars. The arms show a bluer tint, suggestive of ongoing star formation. The bulge is moderate in size. The galaxy displays no signs of being strongly disturbed or merging with another galaxy, although there are indications of minor disturbance. The galaxy is observed face-on. 
