The galaxy presents as a near edge-on spiral, with an apparent dust lane visible along its major axis, obscuring some of the galaxy's light. The galaxy exhibits a relatively smooth disk component with a high degree of rotational symmetry. The bulge is not particularly prominent but appears boxy in shape. There are no indications of active galactic nuclei activity or strong ongoing star formation, as the color appears to be redder, suggesting a relatively older stellar population. No signs of tidal tails or morphological disturbances are apparent, suggesting no recent major mergers or interactions. Overall, the galaxy appears to be a relatively undisturbed and evolved spiral galaxy.
