The galaxy presents as an edge-on spiral. The disk appears relatively smooth, exhibiting minimal visible dust lanes or prominent star-forming regions. There is a slight bulge, which seems to be rounded in shape. The galaxy exhibits no obvious signs of recent or ongoing major merger activity, though minor tidal disturbances or interactions are not entirely ruled out given the resolution. Overall, the system appears relatively quiescent, with low levels of star formation. The galaxy appears to be of considerable mass and absolute magnitude.
