The galaxy presents a somewhat disturbed morphology. There is evidence of a central bulge region appearing bright and relatively smooth. Surrounding the bulge, a less defined, disk-like structure is visible, although it lacks clear spiral arm features. The overall color is slightly blueish, suggesting some ongoing star formation, but there is also a region that has a very yellow/orange appearance, possibly implying an older stellar population and little to no active star formation in that particular part of the galaxy.

There is a distinct asymmetry to the overall galactic structure, with the possibility of a minor interaction or merger event occurring. This is most apparent due to the off-center region.
