The galaxy presents as a relatively faint, elongated object, likely a spiral galaxy viewed nearly edge-on. A central bulge is visible, exhibiting a yellowish-white hue, suggesting a population of older, cooler stars. The disk appears thin and somewhat diffuse. Hints of dust lanes are present near the central bulge along the disk, obscuring some of the starlight. There may be a minor interaction or disturbance evident. While the main structure appears relatively undisturbed, there's a slightly irregular feature or plume extending from one side. The galaxy exhibits a moderate redshift, indicating it is at a significant cosmological distance. Overall, the galaxy seems to be a mid-mass, disk-dominated system with a low star formation rate.
