The galaxy presents as a centrally concentrated object, with a smooth appearance. The main body exhibits a roughly elliptical shape, tending towards circularity, without apparent spiral arm structures or a prominent disk. There is a slight elongation visible, but it is not pronounced. The galaxy's light profile appears relatively uniform, with a gradual decrease in intensity from the core outwards. The overall color of the galaxy appears to be slightly reddish, suggesting an older stellar population or a higher degree of dust obscuration. There may be a minor, faint disturbance or tidal feature visible in the halo region, though it is not very pronounced. There is no clear indication of an ongoing major merger or significant morphological disruption.
