The galaxy appears to be an elongated, disk-shaped structure, viewed at a significant angle. A central bulge is visible, exhibiting a smooth, concentrated light distribution. Moving outwards from the center, the disk shows a fuzzier, less defined structure. There is little evidence of strong spiral arm structure, rather a general, more amorphous distribution of light. The color distribution suggests a possible variation in stellar populations, with bluer hues dominating the outer regions of the disk, potentially indicating areas of more active star formation. A slight warping is visible on the disk. There may be some evidence of tidal disturbances, but further analysis is needed.
