The galaxy presents as a relatively smooth, elliptical object. Its light profile appears diffuse, lacking prominent spiral arms or a well-defined central bulge. The color index suggests a population of older stars, exhibiting a redder hue, with a small amount of recent star formation as suggested by some blue wavelengths of light. There are no significant indications of tidal disturbances or ongoing mergers with other galaxies. The overall morphology indicates a relaxed system. Its approximate diameter is around 3 kpc.
