The object is a disk galaxy, presented edge-on to our line of sight. The central bulge appears prominent and is elongated, indicating a bar structure could be present but obscured by the orientation. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The disk is relatively thin and displays some bluer regions at the periphery indicating ongoing or recent star formation. There are no immediately obvious signs of a major merger or significant tidal disturbances, though subtle asymmetries might indicate a minor interaction. The galaxy appears relatively smooth, lacking well-defined spiral arms. Dust lanes are not distinctly visible, but subtle obscuration effects suggest the presence of dust within the disk.
