The galaxy presents as a spiral type with a discernible disk. The spiral arms are well-defined, displaying a somewhat tightly wound morphology. There is evidence of patchiness along the arms, suggestive of active star formation regions. A central bulge is present, appearing moderately sized relative to the disk. The galaxy is not observed edge-on, and there is no indication of a prominent bar structure. The overall appearance suggests it has not undergone any recent major mergers, although it may have experienced minor disturbances in the past. The color profile suggests ongoing star formation within the galaxy.