The galaxy presents as a spiral type, exhibiting a flattened disk structure. Its arms are moderately defined and appear to wind in a somewhat coherent pattern, revealing at least two distinct arms.  A central bulge is discernible but does not dominate the overall structure. There's no obvious bar feature bisecting the bulge. The overall color profile suggests a spiral galaxy with ongoing star formation.  No major signs of recent or ongoing merger activity are apparent, though there may be minor disturbances. The disk is oriented close to face-on with respect to our line of sight, allowing clear observation of its spiral structure.
