The galaxy presents as a smooth, elliptical shape, with a high degree of central concentration. The light is dominated by a bright, relatively uniform core. A subtle color gradient is observed, transitioning from a slightly bluer hue in the central regions to a redder tone in the outer halo. There is no evidence of distinct spiral arms, dust lanes, or prominent star-forming regions. The galaxy exhibits a lack of significant disturbances. The morphology suggests a passively evolving system, with a substantial population of older stars.
