This galaxy exhibits an elliptical morphology, appearing generally smooth and rounded in shape. Its color profile suggests a population dominated by older stars, with a redder hue indicative of lower star formation rates. There is no discernible spiral structure or distinct disk component. The light appears concentrated towards the center, but the outer regions are still visible. There is evidence of a possible minor disturbance or merger event, the system seems to be composed of two or more galaxies merging with one another.
