The galaxy presents a flattened, elongated morphology, potentially indicative of a disk galaxy viewed at an angle. The central region exhibits a brighter, more concentrated luminosity, possibly representing a galactic bulge or core. There is subtle color variation across the galactic body, suggesting differences in stellar populations. A portion of the galaxy shows hints of bluer hues, perhaps indicating areas of recent or ongoing star formation. The overall structure appears relatively smooth, with a noticeable lack of prominent spiral arms or irregular features. There is a minor visual disturbance in the galaxy's structure, possibly due to a past minor merger event. 
