The galaxy presents as a generally smooth, elliptical object. A bright, concentrated central bulge dominates the morphology. There is a gradual falloff in luminosity from the center outwards. Faint blue-ish outer regions are visible, indicating the presence of a younger stellar population relative to the bulge, but these regions appear subdued, with a lack of sharp or distinct spiral arm features. There appears to be minimal disturbance in the overall shape; it is not undergoing a major merger.
