The galaxy presents a generally elliptical morphology, with a high degree of central concentration. The light profile appears smooth with a notable lack of distinct features such as spiral arms or a prominent bar. Color gradients suggest a centrally concentrated population of older stars, indicated by the yellowish hue dominating the core region. There's a subtle radial decrease in surface brightness outward from the core, blending into a fainter, bluer halo. No evidence of ongoing major mergers or significant tidal disturbances is apparent in the image. The overall appearance suggests a relatively evolved system.
