The observed galaxy presents as a highly inclined, nearly edge-on disk galaxy. There appears to be a prominent central bulge, possibly exhibiting a somewhat rounded morphology. The disk is well-defined, with a smooth, relatively featureless appearance. The color gradient along the major axis suggests potential differences in stellar populations, with bluer colors towards the outer regions of the disk. There may be a slight warp visible, indicating possible gravitational interactions with surrounding galaxies. No prominent dust lanes are readily apparent in this image. Analysis of merging data reveals that the galaxy is likely not undergoing any major merging events. The estimated size of the galaxy is approximately 4.8 kpc. Further spectroscopic data would be needed to confirm any ongoing star formation activity.
