The galaxy presents as a moderately bright, elliptical form. Its overall hue suggests a population of older stars, with a reddish tint dominating the light emitted. The concentration of light towards the center indicates a prominent bulge. The galaxy has a relatively smooth appearance, lacking the distinct spiral arm structures associated with disk galaxies. There is a slight elongation to its shape, deviating somewhat from a perfect sphere. No obvious signs of active galactic nuclei activity are evident. Faint disturbances hint at a possible interaction with a smaller companion in the past. It is likely a massive galaxy, based on its luminosity and size.
