The galaxy appears as an elongated, edge-on disk galaxy. The disk appears relatively smooth with a slight bulge in the center. There is no clear evidence of spiral arm structure or prominent dust lanes within the disk. The galaxy appears to be relatively isolated and undisturbed, with no obvious signs of a major ongoing merger or tidal disruption. Overall, the galaxy has a symmetrical, well-defined structure suggesting it is a fairly mature and undisturbed system. There are no obvious knots of star formation within the galaxy. The galaxy appears to be relatively distant, with a slightly redshifted color profile. 
