The galaxy appears to be an elliptical galaxy, characterized by a smooth and centrally concentrated light distribution. It exhibits a largely featureless morphology, lacking prominent spiral arms or a well-defined disk structure. The galaxy has a round shape, with only a slight deviation from perfect circularity. There is no apparent evidence of ongoing mergers or significant tidal disturbances in the immediate vicinity. The color profile suggests a population of older stars, indicating relatively low ongoing star formation. The galaxy is approximately 7.7 kiloparsecs in radius.
