The galaxy presents as a centrally concentrated object with a high degree of radial symmetry. It appears largely smooth in texture, lacking prominent spiral arms or other distinct features. Its morphology seems closer to elliptical. The color profile indicates a generally redder population. The light distribution suggests a centrally dominant structure, possibly a bulge or a core. There is no evidence of on-going major mergers or significant tidal disturbances in this image. A small hint of a surrounding halo of older stars is possible, but not definitive. The galaxy's overall appearance suggests it is a relatively evolved system.
