The galaxy presents a generally smooth, elliptical morphology. It exhibits a central bulge with a concentrated, luminous core. The light distribution appears relatively uniform, fading gradually from the core outwards. The galaxy shows a slight ellipticity, elongated along one axis. There's little indication of spiral arm structure or significant dust lanes. Its color profile suggests a higher concentration of older stellar populations, and its active star formation rate appears to be low. There is no obvious sign of any merger activity and the morphology is generally undisturbed.
