The galaxy appears as a centrally concentrated object with a generally elliptical morphology. It exhibits a smooth, diffuse light distribution. The central region is notably brighter and has a yellowish hue, suggesting an older stellar population. There is some slight blue tinged coloring toward the outer regions, suggesting possible star formation. There is no obvious evidence of strong spiral arm structures or a prominent dust lane from this view. Overall, the morphology appears undisturbed, with no immediately apparent signs of major interactions or mergers.
