The galaxy presents as a relatively smooth, centrally concentrated object with an overall elliptical shape, nearing circular. The central region exhibits a high degree of luminosity, suggesting a dense stellar population or the presence of an active galactic nucleus. The luminosity fades gradually towards the outer edges of the galaxy. There is a subtle hint of a disk-like structure, though it is not clearly defined, lacking prominent spiral arms. The galaxy does not show any obvious signs of major mergers or tidal disturbances; however, there might be a minor perturbation in its form. The bluer colors suggest some ongoing star formation within the galaxy, albeit perhaps at a moderate rate. Overall, the galaxy appears to be a mature system.
