The galaxy presents a moderately inclined disk, exhibiting prominent spiral arm structure. These arms are somewhat loosely wound and appear to be bifurcated with some degree of branching. The central bulge is of moderate size relative to the overall galactic disk. The galaxy's color profile suggests an older stellar population within the bulge, grading to bluer hues in the spiral arms, indicative of on-going star formation. There is no obvious evidence of a strong bar feature bisecting the central bulge. The morphology displays no indications of major merger events, though some minor disturbances in the disk's symmetry cannot be ruled out.
