The galaxy presents as a smooth, elliptical structure with a concentrated central bulge that appears to be slightly elongated along its major axis. The core exhibits a yellowish hue, likely indicative of an older stellar population. Moving outwards, the galactic halo transitions to a more bluish tint on one side. There are no obvious spiral arms or distinct dust lanes visible. The overall morphology suggests a relatively evolved system with a substantial spheroidal component. There is a slight indication of minor disturbance visible in the outer halo, but the galaxy appears relatively settled.
