The galaxy presents as a somewhat elliptical structure with a smooth appearance. The central region exhibits a bright, concentrated bulge, transitioning outward to a more diffuse disk. There is a slight asymmetry, potentially indicating an interaction or merger event in its past. The color gradient suggests a population of older stars, trending towards redder hues, and a more limited amount of ongoing star formation. The overall light distribution indicates a galaxy with a relatively high Sérsic index.
