The galaxy presents as a flattened, elongated structure, suggesting an edge-on or nearly edge-on disk galaxy. The central region exhibits a concentration of light, potentially indicative of a bulge. A distinct color gradient is observed; the core appears reddish/yellowish, while the outer disk shows a bluer hue. This color difference may imply a difference in stellar population, with the central bulge containing older, redder stars and the disk having younger, bluer stars potentially within ongoing or recent star-forming regions. There may be some slight distortion or a minor disturbance observed along the main axis of the galaxy, but overall, it exhibits a relatively smooth appearance. Based on its color and morphology, it may be undergoing a moderate amount of star formation. Overall, the galaxy appears to be a relatively massive system.
