The galaxy presents an overall elliptical morphology, appearing as a smooth, centrally concentrated light distribution. The core exhibits a yellowish hue, suggesting an older stellar population dominated by evolved stars. Fainter, bluer light extends from the core, hinting at the presence of a disk component. The galaxy's overall shape is somewhat elongated, with an axis ratio deviating slightly from perfectly circular. There is a subtle indication of some minor disturbances, possibly due to a past interaction with another galaxy. There is no clear evidence of strong spiral arm structures or a prominent central bar.
