The galaxy presents as a spiral with well-defined arms. The arms are traced by what appears to be active star forming regions. The galaxy exhibits a bar structure. The central bulge is apparent, but not overly dominant. The overall shape is elliptical, with a major to minor axis ratio of approximately 0.3. The galaxy is inclined relative to our line of sight. There is no evidence of any major merger activity and minimal apparent disturbance of the disk.
