The galaxy presents as a moderately luminous object at a redshift of approximately 0.127. It displays a distinct disk-like structure oriented edge-on relative to our line of sight. The central bulge appears prominent and concentrated, exhibiting a relatively smooth texture.  The disk itself shows signs of internal structure, possibly including dust lanes or spiral arm segments, though resolution is insufficient for definitive identification. There is evidence of potential tidal interaction or recent merger activity, exhibited by asymmetrical light distribution above the disk. The galaxy demonstrates signs of star formation.
