The galaxy presents as a lenticular or edge-on spiral, exhibiting a relatively smooth morphology. A central bulge is discernible, displaying a yellowish hue, suggesting an older stellar population. Extending outwards from the bulge is a faint, elongated disk. The disk shows subtle color gradients, with a bluer tint indicating ongoing or recent star formation regions. The disk appears relatively undisturbed, lacking any obvious signs of major mergers or tidal interactions. Faint dust lanes are suspected within the disk, but are not clearly visible. The overall structure suggests a galaxy that is transitioning from a spiral to a more quiescent state. 
