This galaxy presents as an edge-on spiral galaxy. The central bulge is prominent and appears yellowish-orange, suggesting an older stellar population with lower star formation activity. A dust lane is not obvious, but based on the angle, this would be hard to observe. The spiral arms are tightly wound and bluer in color, indicative of younger, hotter stars and ongoing star formation. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions. The overall morphology suggests a galaxy that is transitioning from a more active star-forming phase to a state of quiescence.
