The galaxy presents as a spiral type, though the structure appears somewhat flocculent and ill-defined, potentially indicating interactions or recent star formation activity.

The central bulge exhibits a moderate size relative to the overall galactic disk, showing a yellow-white hue, suggestive of an older stellar population within the core. The spiral arms are faintly blue, indicating regions of active star formation with younger, hotter stars. There appears to be no strong central bar. The galaxy disk does not appear to be edge-on, rather it is viewed close to face-on.

There are no obvious signs of recent major merger activity, though the arm structure could indicate some minor interaction.
