The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is minimal evidence of spiral arm structure or significant star formation regions discernible at this resolution. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue. The galaxy appears relatively undisturbed, lacking obvious signs of recent major merger activity or tidal interactions. A subtle elongation is present, suggesting it is not perfectly spherical, with the isophotes appearing moderately flattened. It is relatively compact, with a fairly high surface brightness. There is some evidence that there is a very faint disk galaxy extending away from the main body, but this is hard to tell with this image.
