The galaxy presents a primarily smooth, elliptical morphology. There appears to be a bright, concentrated central bulge. The overall color profile suggests a population dominated by older stars, potentially with ongoing, but relatively low, star formation. The galaxy exhibits a slightly elongated shape, displaying no clear spiral arm structure. The outer edges of the galaxy fade gradually, indicating a smooth transition from the main body to the intergalactic medium. There may be minor tidal disturbances present, suggesting a possible past interaction or merger event, but this is not definitive from the image alone.
