The galaxy presents as a face-on spiral with discernible spiral arm structure. The arms are not tightly wound, displaying a relatively open morphology. The central bulge appears prominent, occupying a notable fraction of the galaxy's overall diameter. The disk is relatively smooth in appearance but the arms are clumpy. There's some indication of a bar feature bisecting the central region, though it appears indistinct. The color gradient suggests active star formation within the spiral arms, as evidenced by bluer regions, while the central bulge shows a more yellowish hue, indicative of an older stellar population. There are no obvious signs of a recent major merger or significant tidal disturbance, although subtle asymmetries may suggest minor gravitational interactions.
