The observed galaxy presents a distinct spiral morphology. The spiral arms are well-defined and exhibit a moderate winding, suggesting an intermediate stage of galactic evolution. The central bulge appears relatively small, but it is still quite prominent. Evidence suggests that the galaxy is currently undergoing a minor disturbance, potentially due to a minor gravitational interaction with another galaxy. A weak bar structure may be present within the central region, subtly influencing the arm structure. The spiral arms appear to be composed of two main arms, and a moderate amount of star forming regions, indicating ongoing star formation. The overall color suggests a mixture of stellar populations, with both older, redder stars, and younger, bluer stars contributing to the overall emission.
