The object appears to be a relatively small, distant galaxy. It exhibits a flattened, elongated morphology, possibly indicating an elliptical or lenticular classification, but could also be a highly inclined spiral. The light profile suggests a smooth, centrally concentrated structure with a gradual falloff in surface brightness towards the edges. There is a faint, subtle blueish tinge in the galaxy's core, hinting at the presence of younger stellar populations, although this is not especially distinct, indicating low current star formation rates. The galaxy does not show any obvious signs of tidal interactions or major disturbances, although a minor interaction cannot be fully ruled out given the image resolution.
