The galaxy presents as a moderately luminous object with an overall elliptical morphology. A concentrated central bulge is apparent, displaying a yellowish-orange hue, suggesting a population of older, cooler stars. The light from the bulge decreases in intensity away from the center. The galaxy appears elongated and cigar shaped with some minor disturbances apparent, suggesting it is possibly undergoing interactions or a minor merger. There is some presence of bluer light at the periphery of the object. The galaxy presents with no distinct spiral arm structure, and appears relatively smooth.
