The galaxy presents a mostly smooth, elliptical morphology. It exhibits a bright, concentrated central bulge with a yellowish-red hue, suggesting an older stellar population and minimal ongoing star formation within the core. The outer regions appear more diffuse and slightly elongated, with hints of a fainter, bluish component potentially indicating the presence of younger stars or regions of more active star formation in the disk. The overall structure lacks any strong spiral arm features or signs of major tidal disturbances, indicating it is likely an isolated galaxy that is not currently merging with another galaxy. The roundness of the galaxy is moderately elliptical.
