The galaxy presents as a centrally concentrated object, exhibiting a smooth and largely featureless morphology. The light profile appears to be relatively uniform, with a gradual decrease in intensity from the core outwards. The shape is generally round. There is a slight hint of elongation, but the overall impression is one of high sphericity. No spiral arms, bars, or distinct morphological features are discernible at this resolution. The color is generally yellow, suggesting an older stellar population and a relatively low rate of ongoing star formation. There is no evidence of any major mergers or tidal disturbances, which would present as distortions in the shape or extensions of light.
