The galaxy exhibits a spiral structure. Distinct spiral arms are visible, extending from a central bulge. The bulge appears moderate in size and exhibits a yellowish hue, suggestive of an older stellar population. The spiral arms themselves display a bluer color, indicating the presence of younger, hotter stars and ongoing star formation. There may be some disturbance in the spiral arm structure, though it is not severely distorted. There is no strong central bar. The galaxy disk is face-on. 
