The galaxy presents as a centrally concentrated elliptical-like structure with a smooth, relatively featureless morphology. The light distribution suggests a spheroidal shape, showing a high degree of radial symmetry. There is a noticeable color gradient, with a yellow-orange core indicative of an older stellar population, transitioning to a bluer halo. This suggests some ongoing, albeit low-level, star formation in the outer regions. Overall, the galaxy appears largely undisturbed, showing no signs of major merger activity or significant tidal interactions. There are no obvious spiral arms or a prominent disk.
