The galaxy appears to be a relatively smooth, disk-like system seen at a high inclination. It exhibits a flattened, elongated shape with a discernible central bulge that appears somewhat brighter than the rest of the disk. The disk itself shows a subtle color gradient, with a hint of bluer hues in the outer regions, potentially indicating younger stellar populations and ongoing star formation. Patches of red are present on either side of the center along the disk, suggesting areas of dust obscuration or potentially older stellar populations. There is no strong evidence of spiral arm structure or significant tidal disturbances, suggesting it is likely a relatively undisturbed system that is not undergoing any major merging events. Overall, the galaxy presents as a moderately luminous, rotationally supported system with signs of continued, albeit possibly subdued, star formation.
