The galaxy presents as a spiral type, viewed at an oblique angle. Two dominant spiral arms are discernible, though somewhat indistinct. The winding of the spiral arms appears to be of medium tightness. A central bulge is evident, seemingly of moderate size relative to the overall galactic disk. Indications suggest a possible bar structure, extending across a fraction of the galaxy's diameter. No major disturbances are apparent that would signify a recent or ongoing merger event, although very minor irregularities cannot be ruled out at this resolution.
