The galaxy presents as a relatively compact, disk-shaped structure seen at a near edge-on inclination. The central bulge exhibits a bright, concentrated luminosity. The disk appears slightly asymmetric, with a hint of spiral arm structure discernible despite the inclination. Areas of blue coloration are present in the disk, suggesting regions of recent star formation. The dust lanes are subtle, obscuring some areas of the disk. There is no obvious evidence of a major merger or significant tidal disturbance.
