The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge that emits light in the yellow/orange spectrum, suggestive of an older stellar population. Surrounding the bulge is a more diffuse disk or halo. The disk is a faint blue hue, possibly indicating the presence of younger, hotter stars and ongoing, albeit low, star formation. The overall shape appears to be mostly circular, with a minor elongation. There is no obvious evidence of major disturbances or merging activity, although there may be minor distortions in the outer regions of the galaxy.
