The galaxy presents as a disk-shaped structure, observed nearly edge-on. A prominent bulge is evident, exhibiting a rounded morphology. The disk shows evidence of internal structure and features, potentially spiral arms, as indicated by variations in color and luminosity across the disk. These features are not sharply defined, but their presence suggests ongoing star formation. There is no strong indication of a major ongoing merger, although subtle disturbances or asymmetries are visible in the disk, suggesting a possible minor interaction. The galaxy exhibits a relatively smooth overall appearance, with a small fraction of the light attributed to clumpy, irregular features or artifacts. The galaxy's color profile suggests a mix of stellar populations, with the bulge appearing redder and the disk displaying bluer regions.
