The galaxy presents as an elliptical morphology, appearing largely smooth and rounded in form. It exhibits a concentrated central bulge that graduates into a less defined halo of stars. The color gradient across the galaxy suggests an aging stellar population, with the central region displaying a yellowish hue indicative of older, less active stars. There is a minor disturbance in the galaxy's form, either a slight asymmetrical appearance or a potential tidal interaction with another galaxy. The absence of clear spiral arms or dust lanes suggests the galaxy has a low star formation rate.
