The galaxy appears to be a relatively compact elliptical, characterized by a smooth, featureless morphology. Its overall color suggests a dominance of older stellar populations, implying a low rate of ongoing star formation. The shape approximates a rounded form, with minimal deviation toward a cigar-like or flattened appearance. There is no obvious indication of major mergers or significant tidal disturbances. A slight asymmetry could be due to minor internal structures, but the dominant impression is of a well-relaxed system.
