The galaxy presents as an edge-on spiral, its disk oriented nearly perpendicular to the line of sight. The central bulge is prominent, exhibiting a yellowish-orange hue, potentially indicating an older stellar population. The disk appears relatively thin, showing hints of dust lanes obscuring the starlight along the plane. There is faint blue light visible in the outer regions of the disk, suggesting some ongoing star formation. The galaxy's overall structure appears relatively undisturbed, with no major signs of tidal interactions or significant morphological distortions. A slight boxy shape is observed at the bulge.
