The observed galaxy presents as a spiral galaxy with tightly wound arms. The disk component is dominant, exhibiting a clear, though somewhat disturbed, spiral structure. Star formation appears active within the spiral arms, implied by the somewhat bluer color, though it looks like there is very little in the center, which is a more yellow hue. A distinct bulge component appears to be present, though the exact morphology is difficult to discern. There is a potential disturbance evident in the disk, which could be indicative of a minor interaction or merging event. Overall, the morphology suggests a well-defined, late-type spiral galaxy with ongoing star formation.
