The galaxy presents as a spiral galaxy with a notable disk structure. The arms appear well-defined and exhibit a clumpy texture, suggesting active regions of star formation. The spiral arms seem somewhat flocculent, but are still easily visible. A central bulge is present, appearing relatively small compared to the overall disk size. There is a hint of a bar-like structure across the bulge of the galaxy, as well. The galaxy is viewed at an angle that is less than edge on. The color gradient across the galaxy suggests a radial distribution of stellar populations, with bluer hues potentially indicating younger stars in the spiral arms and a slightly redder hue in the bulge, indicative of older stellar populations. The overall structure is fairly symmetric, though a possible slight asymmetry might be indicative of a minor interaction or disturbance.
