The galaxy presents as a spheroid with a smooth, largely featureless morphology. It exhibits a high degree of central concentration, characterized by a bright, prominent core region which fades smoothly toward the outer edges. No distinct spiral arms or bar structures are discernible. The color profile suggests a population of older stars; it is generally yellow, indicative of evolved stellar populations, potentially with limited ongoing star formation. There is no evidence of any significant tidal features, obvious mergers, or distortions in the overall shape of the galaxy. The overall structure is symmetric.
