The galaxy appears as an elongated, edge-on spiral system. Its overall color is a warm yellow to orange, suggesting a population of older stars with ongoing star formation. There is a subtle color gradient, transitioning towards bluer hues at the outer edges, indicative of the presence of younger, hotter stars in those regions. A central bulge dominates the structure, appearing relatively smooth and concentrated. The disk component is clearly visible, with a high inclination relative to our line of sight. There is no apparent evidence of major mergers or tidal disturbances. The morphology suggests a galaxy undergoing active star formation within its disk, likely a later stage spiral galaxy which has had time for its stars to move towards an older population. 
