The galaxy appears to be relatively smooth and elliptical in shape. Its core exhibits a bright, concentrated luminosity with a yellow hue, suggesting a substantial population of older stars. The light falls off rather quickly from the center indicating a dense core. There may be some minimal indication of a very slight disk component. The morphology indicates a low probability that the galaxy is undergoing any major interaction. Very slight irregularities or disturbances may be present, although they are subtle. Overall, the visual characteristics suggest the galaxy is well-formed, relaxed, and dominated by an older stellar population.
