The galaxy presents an elliptical morphology. The central region exhibits a bright, concentrated core, potentially indicative of an active galactic nucleus or a high concentration of stars. A diffuse, bluish halo surrounds the core, suggesting the presence of a population of relatively young, hot stars or scattering from dust. There is a ring like structure consisting of areas of redder color that could indicate the existence of an older stellar population, dust, or areas of ongoing star formation that have not reached higher temperatures. The galaxy appears mostly smooth, with no obvious spiral arms or strong tidal features. The color gradient transitions from the bluer halo to the redder ring like structure. The overall structure is elliptical, appearing largely undisturbed.
