The galaxy appears to be a spiral type, observed face-on. It exhibits a central bulge which appears relatively small in size and bright. From the bulge, spiral arms emanate outwards. There appears to be three to four arms visible. These arms are tightly wound around the galactic center. There is evidence of ongoing star formation within these arms, as indicated by the blueish hue in the arms. No obvious bar structure is apparent. There is no indication of any major merging activity or significant disturbances.
