The galaxy presents as a disk galaxy, seen nearly edge-on. The disk appears relatively thin and elongated. A prominent central bulge is visible, exhibiting a somewhat rounded morphology. There is evidence of a subtle boxy shape to the bulge, however this may be an optical illusion due to the disk's profile.

The galaxy appears to be relatively smooth in structure, with no prominent spiral arms or distinct star-forming regions readily discernible in the image. There is some asymmetry in the disk. The lack of clear features suggests a relatively quiescent star formation rate. 

There is no strong evidence of a recent major merger or significant tidal interaction that could have disrupted the disk's morphology. However, there seems to be a minor disturbance in the disk, possibly the result of a minor merger event.
