The galaxy presents as an elongated, edge-on spiral. A prominent central bulge is visible, exhibiting a yellowish hue suggestive of an older stellar population. The galactic disk appears relatively thin, with a faint blue tinge towards the edges, which may indicate regions of recent or ongoing star formation. The overall structure suggests the absence of any significant ongoing merger events or major tidal disturbances, although some subtle asymmetries cannot be ruled out without further investigation. Dust lanes are likely obscuring parts of the disk.
