The observed galaxy appears to be a disk galaxy, though its structure is somewhat perturbed. The central region exhibits a bright, concentrated core, with a slightly irregular morphology. This core shows a distinct, concentrated bluish color indicating ongoing star formation. A disk-like structure extends outwards from the core, but this disk does not appear completely smooth or uniform. There is an indication of some disruption or minor tidal features on the edges of the disk. The disk region is multi-colored, displaying a mixture of blue and green tones, consistent with the presence of both young, hot stars and older stellar populations. Redder regions are present near the outer parts of the structure, hinting at possible dust lanes or older stellar populations. Overall, while the galaxy is generally disk-shaped, there are signs of disturbances or interactions that have influenced its morphology.