The galaxy presents as a moderately inclined, disk-shaped structure. There's a distinct blue tint suggestive of recent or ongoing star formation activity. The central region exhibits a yellowish hue. It appears elongated and possibly slightly disturbed, though there is no clear sign of a major ongoing merger, there may be minor disturbances. Dust lanes are not clearly visible, the system is viewed nearly edge-on. The overall morphology suggests a spiral or lenticular galaxy viewed from an angle, possibly undergoing mild interaction.
