This galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge region that appears quite luminous, indicative of a high stellar density. The overall colour is yellowish orange, suggesting a population of older, redder stars dominates its stellar content. There is little evidence of spiral arm structure or significant dust lanes. A smaller, fainter object is located close to the main galaxy, appearing connected by some dim light to the larger galaxy. This object could be another galaxy or a region of active star formation within the same galaxy, or even potentially a tidal tail caused by gravitational interactions.
