The galaxy presents as a disk-like system, observed at a near edge-on orientation. It exhibits a bright central bulge that appears relatively smooth and concentrated. The disk component shows subtle color variations, transitioning from a bluer hue in the outer regions to a slightly redder tone closer to the central bulge. There are faint hints of substructure within the disk, potentially indicating spiral arm segments or dust lane features, though the resolution limits detailed analysis. The overall light distribution suggests a relatively high degree of symmetry and minimal signs of major ongoing merger activity.
