The galaxy presents as a relatively smooth, centralized object. Its morphology appears largely elliptical, with a high degree of symmetry. There is a hint of deviation from a perfect sphere. The core of the galaxy exhibits a concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. Colors appear to indicate a moderate redshift, corresponding with the overall aging of the stellar population. There are very small indications of a disk. There are no obvious tidal tails or signs of major mergers. The galaxy appears relatively undisturbed and evolved. There is a subtle color gradient, transitioning from the central luminosity to the outer edges.