The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing almost spherical, and is tinged with a yellowish hue suggesting an older stellar population. Progressing outwards from the center, the light diminishes gradually. There is some subtle evidence of a faint, bluish extended halo which may indicate a small population of younger stars or ongoing, low-level star formation. There are no clearly discernible spiral arms or other distinct features indicative of a disk galaxy. The overall shape of the galaxy appears relatively undisturbed, with no obvious signs of a recent major merger event.
