The observed galaxy appears to be a spiral galaxy with a prominent central bulge. Faint spiral arms are visible, exhibiting a two-armed structure. The arms have moderate winding. The central bulge has a yellow color, suggesting an older stellar population and reduced recent star formation in that region. There is evidence of a central bar feature, although it is not distinctly defined. There are no signs of any major merger events. The disk appears to be at a slight inclination relative to the observer's line of sight.
