This galaxy appears to be a relatively bright, early-type galaxy with a smooth, rounded morphology. The light is dominated by an orange hue, which could suggest an older stellar population. There is evidence of a possible merger or some kind of tidal disturbance occurring. The galaxy exhibits two distinct clumps. The main component has the orange hue with some green around it, while the secondary clump displays a reddish color. Based on the colors and smooth overall profile of the main component, it's possible we're observing a galaxy with a substantial bulge component.
