The galaxy appears as an elliptical-type object, exhibiting a generally smooth and centralized light distribution. It possesses a moderate ellipticity, trending towards an intermediate shape between round and elongated. The core region is particularly bright, displaying a concentrated luminosity. While the overall form suggests a lack of prominent spiral arms or other distinct disk features, there is a subtle indication of a possible disturbance in its structure, perhaps hinting at a minor interaction or past merger event. The galaxy has a reddish-yellow hue, potentially indicating an older stellar population, or significant dust obscuration. The overall appearance is of a relatively massive, quiescent galaxy at a considerable distance, with a low star formation rate.
