The galaxy presents as a relatively smooth, elongated structure, exhibiting a high degree of axial ratio. It is oriented approximately along a northeast-southwest axis. A bright, concentrated central bulge is evident, transitioning smoothly to a fainter, extended disk. The disk shows subtle color variations, with bluer hues observed along the periphery, potentially indicating regions of ongoing star formation. Overall, the galaxy appears to be largely undisturbed, with no obvious signs of major mergers or tidal features. The structure is consistent with a late-type spiral galaxy viewed at a steep inclination. 
