The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge with a gradual decrease in surface brightness outwards. The color profile indicates a yellowish-orange hue, suggesting a population of older stars, possibly with a lower rate of ongoing star formation. There's no obvious spiral structure or prominent dust lanes visible, though given the resolution, subtle features might be obscured. The morphology suggests a system that has likely undergone significant evolution, possibly through mergers or accretion events in its past, leading to its current spheroid-dominated structure. Minor disturbances cannot be completely ruled out.
