The galaxy presents a morphology consistent with a spiral type, though its disk appears to be closer to edge-on. The central bulge exhibits a relatively smooth and concentrated light distribution, suggesting an older stellar population and minimal recent star formation within the nuclear region. The disk component shows evidence of some structure, potentially indicating spiral arm features, albeit somewhat faint. The overall color suggests a moderate redshift. There is slight asymmetry in its form, and possibly some evidence of minor tidal disturbance or interactions, but these are subtle. The galaxy's orientation provides limited details, and is moderately bright. 
