The galaxy presents as an elliptical structure, with a high degree of radial symmetry. Its overall form appears quite smooth, lacking the distinct features associated with spiral galaxies. The light distribution is centrally concentrated, exhibiting a gradual decrease in intensity from the core outwards. The color profile suggests a relatively homogenous stellar population, potentially dominated by older stars. There's little evidence of ongoing major star formation regions and no strong indication of active galactic nuclei. Faint wisps may suggest minor tidal disturbances, but the galaxy appears largely undisturbed.
