This galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated core. The light distribution is mostly uniform, with a gradual decrease in intensity from the center outwards. There is little evidence of spiral arms or significant dust lanes. The overall color appears somewhat redder, suggesting a population of older stars and a lower rate of ongoing star formation. The galaxy exhibits a slightly elongated shape, closer to an in between round structure rather than perfectly spherical. There is a subtle hint of some minor disturbance in the outer regions, though it is not a clear indication of a major ongoing merger. Overall, this galaxy is most likely a massive galaxy, not undergoing significant amounts of star formation.
