The galaxy presents an overall elliptical morphology, with a notable central bulge that appears relatively smooth and concentrated. There are hints of a disk-like structure surrounding this central bulge, but they are not sharply defined. The light distribution suggests an older stellar population, indicated by the reddish-yellow hue of the bulge. A subtle blue-ish region appears in the outer disk, possibly signifying recent, lower-level star formation. The galaxy's shape is elongated, leaning towards a cigar-like structure. The galaxy appears mostly undisturbed. The overall symmetry suggests a galaxy that may have undergone mergers in the past, though it is relatively relaxed at present. The galaxy possesses a high mass. Overall star formation is occurring at a moderate rate, relative to its high mass. 
