The observed galaxy presents as a spiral galaxy. The spiral arms appear tightly wound around a prominent central bulge. The bulge exhibits a yellow hue, suggesting an older stellar population, while the spiral arms appear bluer, indicative of younger stars and ongoing star formation. Evidence of a bar structure is subtle, but a slight elongation through the bulge is observed, possibly representing a weak or nascent bar. The disk is viewed at a slight angle, showing it is not precisely face-on. The outer regions appear to have some irregular patches. The overall morphology suggests that this galaxy has not experienced recent major merger events.
