The galaxy presents as a relatively bright, disk-shaped structure with a pronounced central bulge. It appears moderately inclined to our line of sight, allowing for some structural details to be observed.

The central bulge exhibits a smooth, concentrated appearance, suggesting an older stellar population. Surrounding the bulge is a fainter, more diffuse disk. Hints of spiral arms or other features are subtle, with only slight variations in color and brightness hinting at possible underlying structure within the disk.

The overall color of the galaxy is somewhat blue-green. Given the observed morphology and color, the galaxy is likely undergoing moderate star formation activity.

There are no signs of recent major merger events, nor strong tidal disturbances. The galaxy is either an isolated galaxy or has undergone minor disturbance events in the past.
