The observed galaxy exhibits a morphology consistent with a spiral galaxy, viewed at a slight angle relative to face-on. Prominent spiral arms are discernible, exhibiting a relatively tight winding pattern. The central bulge is present but appears relatively small in proportion to the disk. There is no evidence of a strong bar structure within the galaxy. The blueness observed in the spiral arms suggests ongoing star formation. Indications suggest there could be a minor disturbance visible.
