The galaxy presents a largely smooth morphology, appearing as an elliptical system seen at a slight angle. The central region exhibits a high surface brightness, characterized by a yellowish-white hue. Proceeding outward from the core, the galaxy's light gradually diminishes and shifts towards a redder color. The isophotes are somewhat elongated, suggesting a deviation from perfect sphericity, trending towards a cigar shape. There are no prominent spiral arms, dust lanes, or other features typically associated with disk galaxies. The overall impression is one of an evolved stellar population, consistent with a massive elliptical galaxy undergoing little star formation. Marginal disturbances are possible but largely absent, indicating it is not currently undergoing a major merger event.
