The galaxy presents as a spiral galaxy with a notable bulge component. Spiral arms are visibly tightly wound. A bar structure is present, though not prominently. The galactic disk appears relatively inclined to our line of sight. The central bulge exhibits a yellowish hue, indicative of an older stellar population. Disk has visible dust lanes. The galaxy appears relatively isolated, with no obvious signs of a major merger or significant tidal disturbances, although minor disturbances cannot be ruled out.
