The galaxy appears to be a spiral galaxy with a moderate inclination. There is a prominent, but somewhat patchy and ill-defined, spiral arm structure visible. One arm is more tightly wound and brighter than the other, which is less defined. Color variation in the arms suggests active star formation regions, with bluer components indicative of hotter, younger stars. The central bulge appears relatively small and indistinct, exhibiting a yellower hue, possibly due to a population of older stars. There is also a faint blueish streak of light that trails away from the galaxy. Overall, the galaxy exhibits indications of ongoing or recent interactions or disturbances based on its asymmetry and features.
