The galaxy appears as a highly inclined, almost edge-on disk galaxy. A prominent dust lane bisects the galactic plane, obscuring the central bulge and near-side of the disk. The bulge appears moderately sized and somewhat rounded. Faint, diffuse light extends outwards from the central region along the plane of the disk. There is no clear evidence of spiral arm structure and no sign of any major ongoing merger events. The disk appears relatively smooth with minor disturbances potentially present. The galaxy exhibits a noticeable red color index, likely due to dust attenuation and older stellar populations. Based on its observed morphology, it's likely a spiral galaxy with an inclination approaching 90 degrees with respect to our line of sight.
