This galaxy exhibits a primarily smooth morphology, with a notable degree of roundness to its overall shape. There are indications of an ongoing or recent merger event influencing its structure. The light distribution suggests a concentration towards the center, with a more diffuse halo extending outwards. The color profile appears relatively uniform, with a yellowish hue dominating the visual spectrum, indicative of a stellar population that is not dominated by very young, hot stars. The estimated size suggests this is a large galaxy. While appearing mostly smooth, subtle irregularities in the light distribution hint at underlying structural complexities potentially related to the merger.
