The galaxy presents a prominent disk structure. Spiral arms are readily apparent, exhibiting a grand design with a morphology dominated by two spiral arms. The winding of these arms appears to be of medium tightness.

A central bulge is clearly visible, estimated to be of moderate size, with a noticeable bar feature cutting through the bulge region. The bar appears somewhat weak, but is still distinct. 

The color profile suggests active star formation within the spiral arms, with bluer hues indicative of younger stellar populations. The redshift indicates this is a relatively distant galaxy. There is no strong evidence of major mergers, though minor tidal disturbances can not be ruled out.
