The galaxy appears as a flattened, disk-shaped structure, suggestive of a spiral or lenticular type. The central region exhibits a high degree of luminosity, which gradually diminishes towards the outer edges of the disk. The galaxy presents itself as nearly edge-on relative to our line of sight. There may be a bulge but this is hard to resolve due to the image quality and angle. No spiral arm structures are clearly discernible. The colour gradient suggests a centrally concentrated older stellar population, while the outer regions might show bluer hues indicative of younger stars, although this is difficult to confirm without higher resolution data. The overall morphology shows a lack of any major disturbances or interactions.
