The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. It has a round to slightly elongated shape. There is a suggestion of a possible ongoing merger event, or at least interaction, with a smaller galaxy or component, due to the close proximity of a secondary concentration of light nearby. The color profile suggests a population of older stars dominating the light output, with a general red hue and a small amount of green within it.
