The galaxy presents as a spiral type, viewed at a moderate inclination angle, possibly close to face-on. Distinct spiral arm structures are observed, though the arm definition appears somewhat flocculent, lacking sharp, continuous tracing. The central bulge is of moderate size relative to the overall galactic disk. A weak bar structure seems to extend through the core region, contributing to the overall shape of the galaxy. The disk exhibits a relatively smooth texture, with possible active star formation in the spiral arms. Overall morphology does not indicate any signs of on-going major mergers, but some minor disturbance cannot be ruled out.