The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a generally spheroidal morphology. There is minimal evidence of spiral arms or a prominent disk structure within the visible light spectrum. Its color profile suggests a population of older stars, exhibiting a redder hue, indicating a lower rate of current star formation. There appears to be little to no dust or gas visible in this image, which is consistent with a later type galaxy. The galaxy appears well-defined, showing little signs of a major merger event or significant tidal disruption. The object shows a fairly rounded shape. Faint hints of a minor disturbance might be present, but could also be due to image noise. Overall, the galaxy presents as a passively evolving system.
