The galaxy presents as a moderately inclined spiral with prominent, well-defined spiral arms. The arms exhibit a somewhat flocculent structure, displaying numerous bright knots suggestive of active star formation regions. These regions are bluer in color, indicating the presence of young, hot stars. Dust lanes are faintly visible within the spiral arms, particularly on the near side of the galaxy. 

The central bulge appears moderately sized and exhibits a yellowish-white hue. The bar structure within the galaxy is clearly visible, with a somewhat disorganized presentation. The overall morphology suggests a galaxy undergoing active star formation, with some signs of minor disturbances. The color indices indicate a higher luminosity in the r and z bands compared to the g band.
