The galaxy presents an overall elliptical morphology, appearing moderately smooth in texture. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue indicative of an older stellar population. Fainter, bluish extensions are visible surrounding the central bulge, suggesting the presence of a younger stellar population and potentially some ongoing star formation, although at a seemingly low rate. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or major mergers. There is a slight disk-like structure around the center. The overall color profile suggests a galaxy that is transitioning from active star formation to a more quiescent state, although the outer regions may still harbor pockets of younger stars.
