The observed galaxy presents as a spiral galaxy with a slight inclination relative to our line of sight. The disk component dominates the visual structure, exhibiting a moderately wound spiral arm morphology. A small bulge is visible at the galactic center. Patches of blue-tinged regions are irregularly distributed throughout the spiral arms, potentially indicating areas of active star formation. There is no strong evidence of a significant bar structure. The overall appearance suggests a late-type spiral galaxy. No major merging signatures, or clear tidal features are detected, although there is a possible minor disturbance.
