The galaxy presents as a spiral, viewed at a moderately oblique angle. Spiral arms are discernible, although somewhat disturbed or flocculent in nature, emanating from a central bulge. The winding of these arms appears somewhat tight.

The central bulge appears prominent and moderate in size in relation to the overall galactic disk. Dust lanes are also present within the disk and obscuring the bulge region.

There is evidence of interactions or disturbances in the morphology of the galaxy, potentially indicative of a minor merger or tidal disruption.

The disk shows varying degrees of star formation activity, with some regions appearing bluer, suggesting more recent or ongoing star formation, and other regions exhibiting redder hues.