The galaxy presents as a singular, moderately luminous object with a relatively smooth, elliptical morphology. The central region exhibits a bright, concentrated core indicative of a substantial stellar density. Moving outwards, there's a gradual decrease in luminosity. The overall color of the galaxy appears to be in the redder part of the spectrum. No distinct spiral arms, bars, or other significant structural features are discernible. The object appears undisturbed, without any evident tidal tails or morphological distortions suggestive of recent major mergers. Some minor irregularities or faint features may be present in the outer regions but are not clearly resolved at this scale. The overall impression is of a mature galaxy with relatively low levels of on-going star formation.
