The galaxy presents as a slightly elongated, disk-like structure oriented at a significant angle relative to our line of sight. The central region exhibits a relatively smooth, concentrated bulge. The luminosity profile appears to decrease gradually from the bulge towards the outer edges of the disk. Hints of a faint, diffuse halo surround the main body of the galaxy. There is a subtle asymmetry or minor disturbance visible within the disk, suggesting the potential influence of a past interaction or minor merger event. Overall, the galaxy's structure is largely smooth, with only weak evidence of distinct spiral arm features. Its color indices point to moderate ongoing star formation activity. The object is likely a spiral or lenticular galaxy at a considerable distance, judging from its apparent size.
