The galaxy presents as a somewhat elliptical morphology, though not perfectly spherical. A smooth luminosity gradient is observed, increasing towards the central region which appears intensely bright and yellowish-white, suggesting a high concentration of older stellar populations. Fainter, bluish halos surround the central region, implying the presence of some younger stars or ongoing star formation in the outer reaches of the galaxy. Faint disturbances appear to emanate from this galaxy suggesting it may be undergoing a merger or has undergone a recent disturbance.
