The galaxy presents as a centrally concentrated, smooth object with an elliptical morphology. Its light profile suggests a relatively old stellar population. The central region exhibits a pronounced brightness, indicative of a bulge component that could contain a supermassive black hole. The galaxy's light exhibits a redder hue, likely a result of dust content, older stars, or a combination of the two. There appears to be an absence of distinct spiral arms or prominent star-forming regions within this particular image resolution. No obvious tidal features or distortions are visible, suggesting it has not undergone any recent major mergers or interactions.
