The galaxy presents as a spiral type, exhibiting well-defined arms originating from a central bulge. The spiral arms appear relatively tightly wound closer to the center, gradually loosening towards the outer edges. Two spiral arms are strongly suggested. The central bulge appears to be of moderate size compared to the overall galactic disk. There's no clear indication of a bar structure bisecting the bulge. The disk inclination is close to face-on. No obvious signs of major mergers or significant tidal disturbances are observed. The galaxy presents a generally smooth appearance.
