This galaxy presents as an edge-on spiral or lenticular galaxy at a significant cosmological distance. The morphology suggests a relatively high inclination angle with respect to our line of sight, obscuring the spiral arm structure. The apparent size is small, but this is influenced by distance.

The galaxy exhibits a central bulge, which appears somewhat elongated and possibly boxy. A dark dust lane is visible, bisecting the galaxy along its major axis. This suggests the presence of a substantial disk component. The color is dominated by a yellowish/orange hue. The galaxy exhibits ongoing star formation, although the rate appears to be moderate.

There are no obvious signs of a major merger or significant tidal disturbance affecting the galaxy's morphology. Minor disturbances or asymmetries cannot be entirely ruled out, but the overall appearance is relatively quiescent.
