The galaxy presents as a spiral, viewed at a moderate angle, close to face-on. It exhibits distinct, though somewhat loosely wound spiral arms, that extend from a bright, moderately sized central bulge. There appear to be multiple spiral arms. A bar feature is noticeable in the galaxy's center but is obscured by the central bulge. The disk component is prominent and shows an appreciable degree of blue color, potentially indicating active star formation regions. The galaxy's overall shape shows signs of some tidal disturbance or a recent minor merger event, possibly influencing the arm structure. The light distribution appears relatively smooth, with a concentration toward the bulge, but there are also star-forming regions with brighter pockets visible throughout the spiral arms. The galaxy appears moderately inclined, given the elliptical shape of the disk.
