The galaxy appears as a centrally concentrated system with a smooth light distribution, exhibiting a relatively round morphology. There's no discernible spiral arm structure, but instead a more diffuse, elliptical shape. The galaxy's color is predominantly yellowish-orange, suggesting a stellar population dominated by older, cooler stars. There are no visible dust lanes or significant signs of active star formation regions discernible within the image. The core region is bright, with a gradual fading of intensity towards the edges, indicating a centrally dense structure. It appears to be undergoing a merging event, where at least 2 or 3 galaxies are interacting with each other. These galaxies do not have many young stars within them.