The galaxy exhibits a generally smooth morphology. The central region presents a concentrated, yellowish-white luminosity, suggestive of an older stellar population. The galaxy appears to be disk-like, as it is elliptical in shape. Subtle indications of a faint, diffuse, bluish disk or extended halo exist, but the structure is largely smooth. There is no compelling visual evidence of spiral arms or bar features. No signs of a recent or ongoing major merger event are readily apparent.
