The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge exhibiting a yellow-orange hue, indicative of an older stellar population. There is a slight elongation in the structure but it is mostly round in appearance. Faint blue regions can be observed, indicating the presence of some ongoing star formation, although it appears largely quiescent. The system does not display any prominent spiral arm structures or distinct dust lanes, suggesting a relatively evolved system. The galaxy seems to be undergoing or has undergone a merger event, with notable tidal features. Overall, the galaxy appears to be a massive, relatively evolved system with evidence of past or ongoing interactions influencing its morphology and star formation activity.
