The galaxy presents as a relatively compact, elliptical morphology with a smooth, diffuse light distribution.  The central region exhibits a concentrated brightness, suggesting a high stellar density or possibly an active galactic nucleus, though no distinct point source is visible.  There is a subtle color gradient from the core outwards, with the inner regions appearing slightly redder and the outer regions trending towards blue. No spiral arms, bars, or obvious dust lanes are apparent, supporting its classification as an elliptical galaxy. Faint distortions or tidal features are not readily discernible, suggesting the absence of recent major merger events. The overall impression is of an evolved galaxy with relatively low ongoing star formation.
