The galaxy appears to be a spiral galaxy, viewed edge-on. There is a central bulge that is yellow in color, suggesting an older stellar population. Surrounding the bulge, there is evidence of a flattened disk. The disk shows a bluish tint, indicative of ongoing star formation. The galaxy appears relatively undisturbed, exhibiting no strong signs of a recent major merger. However, there may be subtle asymmetry, or minor disturbances present in the outer regions of the disk. The overall light distribution appears concentrated with a relatively smooth, extended profile. The galaxy is of moderate size, with an absolute magnitude corresponding to that of a typical spiral. The star formation rate is also typical, suggesting a relatively normal evolutionary stage.
