This galaxy presents a smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decrease in surface brightness towards the edges. There is no strong evidence of spiral arms or significant dust lanes. The color is subtly redder in the center, indicating a likely concentration of older stars. The overall shape is close to round, with only a slight deviation towards an elongated appearance. There are no obvious signs of recent or ongoing mergers, though some minor irregularities in the outer regions may suggest past interactions. Overall, the galaxy appears as a fairly quiescent, evolved system with minimal ongoing star formation.
