The galaxy presents as an elongated, elliptical structure with a smooth, diffuse light distribution. The core region is bright and concentrated, exhibiting a slightly yellow-white hue. Extending outwards from the core, a fainter, blueish-white halo is visible. There is no strong evidence of spiral arms or dust lanes. The overall morphology suggests a relatively evolved system, possibly an elliptical galaxy or a lenticular galaxy viewed at an oblique angle. The lack of distinct features such as active star-forming regions or tidal tails implies a relatively quiescent state. The galaxy appears to be isolated and does not display signs of major mergers or significant interactions with other galaxies.
