The galaxy presents a generally smooth and rounded morphology. It exhibits a concentrated central bulge with a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy show a slightly bluer color, potentially indicating the presence of some ongoing, though not dominant, star formation. There is no clear evidence of spiral arms or a well-defined disk structure. Minor asymmetry appears, but it does not imply a major merger event; it could be a minor disturbance within the galaxy's structure.
