The galaxy presents as a highly inclined, disk-dominated system viewed nearly edge-on. The dust lane obscuring the midplane is not clearly visible, suggesting either minimal dust content or a relatively smooth dust distribution. The central bulge appears subtle and elongated along the major axis of the disk. Color gradients within the galaxy appear smooth, with the bulge and inner disk region showing a slightly redder hue compared to the outer disk, potentially indicating older stellar populations in the central regions. The disk exhibits a faint, diffuse outer structure. No signs of recent major merger activity or prominent tidal features are detected. The overall morphology indicates a relatively undisturbed system, with its classification likely as a late-type spiral or possibly a lenticular galaxy.
