This galaxy appears to be a relatively bright, disk-dominated spiral system observed at an inclination that is neither edge-on nor face-on. There is a central bulge region that appears quite luminous. It is surrounded by a somewhat diffuse disk. The disk shows hints of spiral arm structure, although the arms are not sharply defined. The color gradient within the galaxy suggests some degree of ongoing star formation, particularly within the disk regions, which exhibit bluer hues compared to the central bulge. The overall morphology suggests a galaxy that is relatively undisturbed, without signs of major merger activity, though there may be some minor disturbances present. The galaxy exhibits a roughly elliptical shape, with a moderate axis ratio. The overall light distribution is fairly smooth, indicating a relatively evolved system, although some clumpy structures are present within the disk, suggesting regions of active star formation.
