The galaxy presents as an edge-on or highly inclined disk galaxy. It exhibits a prominent central bulge that appears relatively smooth and featureless, indicative of an older stellar population dominating this region. The disk itself is elongated and displays a complex structure. One side of the galaxy appears truncated or shows signs of tidal disruption or interaction. There are some indications of ongoing star formation within the disk, with a few regions displaying a slightly bluer hue.  Overall, the galaxy appears to be a relatively massive, actively star-forming spiral galaxy undergoing some form of gravitational interaction or disturbance. 
