The galaxy appears to be a spiral type, viewed at a slight angle but not quite edge-on. The central bulge is prominent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Fainter spiral arms extend outwards from the central bulge. The arms are somewhat fragmented and lack sharply defined structure. There appears to be ongoing star formation in the arms, traced by regions of bluer light. Overall, this galaxy exhibits moderate star formation activity. The dust lanes are not clear. There may be some minor disturbances in the morphology, but no major interactions or merger events are apparent. The overall structure suggests a relatively well-formed disk with a prominent bulge. There is no strong bar structure visible.
