The observed galaxy exhibits a prominent disk structure with a central bulge region. The spiral arms are well-defined. A subtle bar structure appears to bisect the central bulge. Star forming regions, indicated by blue light, are distributed primarily within the spiral arms. A fraction of its light is emitted from a relatively smooth component, indicative of an older stellar population. The morphology suggests a classification as a spiral galaxy. There is some evidence of minor disturbances in the galaxy's structure, perhaps due to minor interactions.
