This galaxy presents as a flattened, elongated structure with an elliptical morphology. The central region exhibits a concentration of light, suggesting a bulge component. The color profile indicates a relatively smooth transition from the core outwards, with a gradual decrease in luminosity. The overall shape appears quite elongated, with hints of spiral structure at the edges. This suggests a possible disk galaxy, viewed at an oblique angle. There may be ongoing star formation indicated by the bluer regions in the outer parts of the galaxy. The lack of distinct, well-defined spiral arms suggests a relatively smooth or flocculent spiral galaxy type. There are possible signs of disturbances. The outer disk appears truncated.
