The galaxy presents as a disk galaxy seen nearly edge-on. There's a prominent central bulge, which appears smooth and has a rounded morphology. The disk exhibits a noticeable dust lane bisecting it horizontally, obscuring some of the light from the bulge and inner regions. The galaxy is characterized by a relatively smooth texture. The light distribution suggests a mature stellar population. There are no readily apparent signs of major ongoing mergers or significant tidal disturbances, though there is a potential slight asymmetry or minor irregularity at the periphery of the disk that could be interpreted as a minor interaction. Overall, the galaxy appears as a relatively undisturbed, evolved system.
