The object presents as a single, relatively compact galaxy. Its morphology appears largely smooth and elliptical, with no readily discernible spiral arms or bar structure. The galaxy exhibits a dominant central bulge that appears roughly circular. Color gradients suggest an older stellar population throughout the galaxy, with a particularly high concentration of such stars in the bulge. There is some minor evidence of disturbance in the galaxy's light profile, but it appears to be overall relaxed, with an estimated effective radius of about 8.7 kpc. Overall, this appears to be a massive, quiescent galaxy with a minimal rate of star formation.
