The galaxy presents as a somewhat elliptical, diffuse object. Its morphology appears primarily smooth, with no readily discernible spiral arm structures or prominent dust lanes. The light profile shows a centrally concentrated core, exhibiting a yellowish-white hue, suggesting an older stellar population or dust obscuration. The outer regions of the galaxy gradually fade into the background sky, indicative of a declining stellar density. There is a hint of bluer light in the outer regions of the galaxy, suggestive of some younger stars or star forming regions, but overall the galaxy appears redder. No obvious signs of tidal disturbances or recent mergers are apparent in this image.
