This galaxy appears to be a relatively smooth object, likely an elliptical galaxy or a lenticular galaxy. It exhibits a moderate central bulge which is apparent from the concentration of light towards the center. The galaxy's shape is somewhat elongated. The lack of distinct spiral arms and the relatively smooth light distribution indicate a more evolved system, potentially with a lower rate of star formation compared to spiral galaxies. There may be a slight disturbance visible in the outskirts, perhaps due to a minor interaction or recent merger. Overall, the galaxy appears to be a fairly massive system located at a moderate distance. The color distribution indicates a population of older stars, especially concentrated towards the core.
