The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely spheroidal, with a noticeable lack of distinct spiral arms or a prominent disk. The central region exhibits a yellowish hue, suggesting an older stellar population. There is a subtle colour gradient visible, transitioning from the yellowish core to a slightly bluer outer halo, hinting at some ongoing, albeit subdued, star formation in the periphery. There is no obvious indication of any major mergers or tidal disturbances. The galaxy appears approximately round in shape, showing minimal elongation.
