The galaxy presents as a singular, luminous object with a generally elliptical morphology. The light is concentrated centrally, indicative of a high stellar density core. The light distribution appears smooth, suggesting a lack of distinct spiral arms or prominent dust lanes. The galaxy exhibits a yellow-orange hue, possibly indicating an older stellar population dominated by redder stars, or significant dust obscuration within the galaxy. No obvious signs of recent major mergers or tidal disturbances are visible. The overall appearance points to a galaxy with a largely undisturbed morphology, possibly an elliptical galaxy or a lenticular galaxy seen at a considerable distance.
