The galaxy presents as a highly elongated, disk-like structure, viewed at an extreme angle. It appears relatively smooth in texture, with a bright, concentrated central bulge that dominates the luminosity profile. The disk exhibits a gradual color gradient moving outwards from the central bulge. The inner regions are generally more blue. There is no evidence of prominent spiral arms. A faint, diffuse halo surrounds the main body of the galaxy, with little indication of significant ongoing star formation. The galaxy appears undisturbed, exhibiting no obvious signs of recent merger activity or tidal interactions.
