The galaxy presents as a luminous elliptical, exhibiting a smooth, centrally concentrated morphology. There is no apparent spiral structure or disk-like features. The isophotes appear generally round, with only a slight deviation towards ellipticity. A gradual decrease in surface brightness extends from the bright core, suggesting a relatively old stellar population and minimal on-going star formation. Minor disturbances in the overall symmetry are present, though they do not suggest a major ongoing merger event. The color profile is largely uniform, with a redder hue indicating an evolved stellar population. The galaxy exhibits a non-negligible angular size, indicative of a substantial physical dimension.
