The galaxy presents as a spiral galaxy with a well-defined disk structure. The spiral arms are moderately tightly wound and exhibit a clumpy morphology, suggesting active regions of star formation. A prominent bulge is observed, occupying a substantial portion of the galaxy's central region, although not dominating it. The bulge appears relatively smooth. The disk extends beyond the bulge, showing spiral structure. There is a hint of asymmetry in the overall structure, possibly indicating a minor gravitational interaction or disturbance. The galaxy's color suggests a mix of stellar populations, with a central yellow hue and bluer regions along the spiral arms.
