The observed galaxy presents as a spiral structure, exhibiting prominent, well-defined spiral arms. These arms are characterized by a clumpy appearance suggestive of active star formation regions, interspersed with darker dust lanes. The galaxy's disk is viewed at a moderate inclination, allowing a clear view of the spiral arm structure.

A small bulge appears centrally, which is not particularly luminous. Evidence suggests a bar may be present, appearing to cross the central bulge. Morphological analysis indicates that the galaxy may be undergoing a minor disturbance or merger, with some asymmetry observed in the outer regions of the disk. The overall color profile indicates an intermediate stellar population, with hints of blue star formation regions within the spiral arms and redder, older stellar populations concentrated toward the central bulge. 
