The galaxy presents as a luminous, elliptical morphology with a centrally concentrated bulge. It exhibits a smooth light distribution, suggesting an older stellar population with minimal ongoing star formation. The galaxy appears elongated, with a moderate axis ratio. There is little evidence of spiral arms or significant dust lanes. The primary color is a yellow-orange hue, possibly indicating a relatively old stellar population, but there is a hint of bluer color in the outer regions, which could indicate some limited star formation activity. No signs of major merger events or tidal disturbances are apparent in the immediate vicinity. Overall, the galaxy appears to be a relatively undisturbed, early-type galaxy.
