The galaxy presents as an elongated, disk-like structure viewed nearly edge-on. A prominent dust lane bisects the galaxy, obscuring the central bulge and parts of the disk. The disk exhibits a noticeable color gradient, transitioning from bluer hues at the edges to a more yellowish-white towards the core. There is no strong evidence of spiral arm structure visible from this perspective. The galaxy appears relatively undisturbed, lacking any major tidal features or signs of recent mergers. The light distribution suggests a relatively smooth stellar population.
