The galaxy presents as a moderately bright, disk-shaped structure with an apparent reddish-yellow hue. It exhibits a smooth, centrally concentrated bulge that dominates the overall light profile. The disk component appears relatively featureless, lacking prominent spiral arm structures or distinct dust lanes in this imagery. The galaxy's morphology suggests a late-type spiral or possibly an early-type lenticular galaxy, with the smooth profile potentially indicating a relatively older stellar population and a lower rate of ongoing star formation. The overall appearance suggests a system that is transitioning from a more active, star-forming phase to a quiescent state.
