The galaxy appears to be a spiral galaxy with a moderately bright central bulge. The spiral arms are somewhat tightly wound and exhibit a clumpy structure, suggesting regions of active star formation. There is some disruption visible in the arm structure, which may be indicative of an ongoing or past minor merger event. The galaxy presents a moderately inclined disk, allowing for observation of spiral structure. There is no clear sign of a strong bar feature. Overall it is a moderately luminous galaxy at moderate redshift.
