The galaxy presents as a somewhat elongated, lenticular structure with a smooth, centrally concentrated light distribution. A bright, concentrated core region emits strongly, indicating the presence of a dense stellar population. The overall color of the galaxy is yellowish-red. This suggests a relatively evolved stellar population with a low rate of ongoing star formation. The halo appears relatively homogenous, with no discernible spiral arm structure or significant dust lanes. Slight asymmetries may indicate a minor gravitational disturbance but appear indistinct. The galaxy is relatively massive based on its size and luminosity, but has a low star formation rate.
