The galaxy presents a distinct spiral morphology. The central bulge appears prominent and moderately luminous, exhibiting a soft, almost diffuse glow. The spiral arms are tightly wound and emanate from the core, exhibiting a fragmented appearance with hints of active star formation. These areas show up as bluer tinges dispersed throughout the arms. The disk is viewed nearly face-on, allowing for a clear view of the spiral structure. There is no significant presence of dust lanes, the disk and arms are slightly warped, but there is no visible evidence of significant tidal interactions with any neighboring galaxies or galactic mergers.
