The galaxy appears to be a relatively smooth, elongated structure. It is likely an edge-on spiral or lenticular galaxy. There is a subtle hint of a central bulge, but no distinct spiral arms are visible. The light distribution is somewhat uniform, lacking prominent knots or regions of intense star formation. The color is predominantly blueish-white, suggesting the presence of a relatively young stellar population, although some of the blue hue may be redshifted. There may be minor distortions in the galaxy's shape, potentially indicating an interaction with a smaller companion. Based on the galaxy's shape and smoothness, it may be experiencing a low rate of star formation.
