The galaxy presents a generally smooth and concentrated morphology, characteristic of an early-type galaxy. It exhibits a bright, relatively spherical central bulge which emits light across the visible spectrum, with a noticeable concentration in the redder wavelengths. The overall shape of the galaxy is elliptical, although not perfectly round. The isophotes appear mostly smooth and regular. Subtle disturbances can be detected, however these are relatively minor. The outer regions appear fainter and bluer than the core, implying a population of younger stars perhaps. The galaxy does not show any prominent spiral arms or a distinct disk structure, which also supports the classification as an elliptical or lenticular galaxy. No strong signs of a major merger event are clearly visible, though some small disturbances may be present.
