The galaxy presents a somewhat elliptical morphology, appearing generally smooth in texture. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer edges. There is a slight elongation evident, however, it is difficult to discern whether it is a true elliptical or a highly inclined spiral galaxy. The color profile suggests a relatively older stellar population, displaying a yellowish-orange hue indicative of evolved stars. There is no indication of substantial dust lanes or active star formation regions in this image. The overall impression is of a quiescent galaxy with a large stellar mass and potentially low current star formation rate.
