The galaxy presents as a relatively smooth, elliptical morphology with a prominent central bulge. The light distribution suggests an older stellar population, particularly concentrated within the bulge, which exhibits a yellowish-orange hue. Fainter, bluer light surrounds the central bulge, suggesting the presence of some younger stars. There is no evidence of spiral arms or significant dust lanes. The overall shape is moderately elongated. There is no apparent active galactic nucleus or interaction with companion galaxies.
