The galaxy presents as an elongated, edge-on or highly inclined spiral system. Its overall color is reddish-orange, indicating a population of older stars and/or significant dust obscuration within the disk. The galaxy appears relatively smooth, lacking prominent, well-defined spiral arms or intense star-forming regions that would be characterized by bright blue knots. There is a slight hint of a central bulge, though the resolution is insufficient to determine its precise morphology. Based on its apparent lack of significant disturbances, it seems to be a relatively isolated system, and not currently undergoing any major merging events. It is likely a large and massive system with a high star formation rate given its high luminosity. 
