The galaxy appears as a single, centrally concentrated object. It exhibits a smooth morphology, lacking any readily discernible spiral arms or a prominent disk structure. The light distribution is relatively uniform, suggesting a lack of significant star-forming regions or dust lanes. The galaxy appears roughly elliptical with an estimated radius of 6.7 kpc. The color is relatively uniform and exhibits a slightly reddish tint. No features that would obviously indicate tidal disturbances or an ongoing merger are apparent.
