This galaxy appears to be a disk galaxy, likely a spiral galaxy observed at a near-edge-on inclination. The central bulge is prominent, exhibiting a yellowish-orange hue indicative of an older stellar population. The disk itself shows a bluer color, suggesting more recent or ongoing star formation activity, though it is not uniformly distributed. One side has a brighter concentration of blue light than the other. There are slight distortions, suggesting the potential for a minor interaction or merger. The morphology suggests an elliptical structure with some disk features.