This galaxy presents as an edge-on disk galaxy. There is a central bulge that appears more luminous with a slight yellowish tint, suggesting an older stellar population. The disk extending from the bulge displays a fainter, somewhat diffuse glow along the galactic plane, with dust lanes likely obscuring some of the starlight. No distinct spiral arm structure is visible, a probable consequence of the viewing angle. Based on the color profile, the galaxy shows evidence of moderate star formation within the disk. There are no signs of any ongoing major merger events or significant tidal disturbances.