The galaxy presents as a luminous, elliptical-like structure, with a concentrated central bulge. The light is generally smooth and appears to be comprised mostly of older stars, with very little evidence of dust lanes or significant star formation regions. The galaxy displays a yellowish-orange hue, consistent with a population of evolved stars. The outer regions of the galaxy fade gently into the background sky, with a fairly smooth and gradual decrease in luminosity. There is a slight elongation in its shape. No spiral arms or other disk-like features are clearly discernable. Overall, the galaxy appears relatively undisturbed, lacking any obvious signs of recent merger activity or strong tidal interactions. The morphology suggests it is likely a fairly massive system.
