The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, although it shows a slight deviation towards a more oblate form, not perfectly round. There's a color gradient, shifting from a yellow-tinged core to a bluer periphery. The core region appears denser and brighter, suggesting a higher concentration of older stars. The outer regions exhibit a fainter, more diffuse light, possibly indicative of younger stellar populations or ongoing star formation. There's no clear evidence of spiral arms or a distinct disk structure. No major disturbances or merging features are apparent.
