The galaxy presents as a spiral galaxy with a clear disk structure, seen at an oblique angle relative to our line of sight. The central bulge exhibits a yellowish-white hue, indicative of an older stellar population. The spiral arms are somewhat tightly wound and display bluer colors, suggesting ongoing star formation. Dust lanes are faintly visible within the disk, particularly on the near side of the galaxy as inferred from the angle of observation. The overall morphology suggests a relatively mature spiral galaxy, but with some evidence of current star formation within its spiral arms. There are possible signs of a very slight merger event or minor disturbance, as evidenced by some asymmetry.
