The galaxy exhibits a prominent disk structure oriented at a slight angle relative to the line of sight. Well-defined spiral arms are visible, tracing out a grand design. These arms are relatively loose and open, extending outwards from a central bulge. The winding of the spiral arms appears to be medium to loose. The central bulge appears moderately sized, with light that gradually fades towards the outer regions of the galaxy. The light in the disk is dominated by blue colors. The spiral arms display clumpy regions, indicative of active star formation. The galaxy shows no strong evidence of any recent or ongoing major merger events, though some slight disturbances may be present. There are some subtle hints of a bar-like structure in the central region of the disk.
