The galaxy appears to be elliptical in shape, exhibiting a smooth, largely featureless morphology. Its color profile suggests a population of older stars. The concentration of light is high toward the center, with a gradual fading towards the outer edges of the galaxy, indicating a centrally concentrated stellar distribution. There is no evidence of spiral arms or a prominent disk structure. The overall appearance indicates a well-relaxed system, with minimal signs of recent mergers or tidal disturbances. The galaxy presents a slightly yellowish hue, potentially indicative of a dominant population of older, cooler stars.
