The galaxy presents a generally smooth and rounded morphology. The light profile appears relatively uniform, with a concentrated central region that gradually fades outwards. The color is suggestive of an older stellar population, with a noticeable yellow-orange hue. There may be some minor internal structure, but the resolution is insufficient to resolve any distinct spiral arms or bar features. There is no obvious tidal debris or indication of recent major merger events. Based on its overall appearance, the galaxy is most likely an elliptical galaxy.
