The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a primarily elliptical morphology, showing little evidence of a distinct disk or spiral arms within this image. There are no signs of ongoing major mergers or tidal disturbances, but there is a slight lopsidedness that may indicate minor gravitational interactions. The color profile suggests a population of older stars, with a subtle hint of more recent star formation activity as well. Overall, this galaxy is a massive, evolved system transitioning away from its star formation phase.
