The galaxy presents a complex, disturbed morphology indicative of ongoing or recent interaction. A central, bright core suggests a concentration of older stars, possibly a small bulge component. Spiral arms are clearly visible, though somewhat irregular and tightly wound close to the core, and of intermediate winding further out. Patches of bluer light suggest regions of active star formation within these arms. Overall, the galaxy appears elongated with its major axis oriented roughly diagonally. Dust lanes appear present, but are not prominent features. The outer regions exhibit a fainter, less defined structure, possibly a stellar halo or tidal debris.
