The galaxy presents as a spiral galaxy with well-defined spiral arms. The arms appear to be tightly wound around a prominent central bulge. The bulge exhibits a moderate size relative to the overall galaxy. The spiral arms display a clumpy morphology, suggesting active regions of star formation. There appears to be ongoing star formation within the galaxy, as indicated by the presence of blue-ish regions in the arms. There are no clear indications of a strong bar structure. The overall color of the galaxy suggests a relatively high stellar population with evidence of both young, blue stars and older, redder populations. There might be minor disturbances due to interactions.
