The observed galaxy presents as an edge-on spiral with a redshift indicating intermediate distance. The disk appears to be relatively thin. Dust obscuration is visible within the plane of the disk, characterized by dark and somewhat irregular bands. A central bulge is apparent, exhibiting a smoothly rounded morphology. There may be a subtle indication of some tidal disturbance or minor interaction. Star formation activity appears present but not exceedingly dominant, consistent with a late-type disk galaxy with moderate star formation rates. No major merging features are discernible, suggesting a relatively isolated system.
