The galaxy presents as a relatively smooth, elliptical morphology. Its light profile suggests a centrally concentrated structure. The color appears somewhat red, indicating a stellar population that is likely older and less actively forming stars. There is little evidence of spiral arm structure or significant dust lanes within the optical wavelengths captured. Overall, the galaxy seems to be a fairly evolved system, with a substantial mass. There is no obvious signs of any on-going major merger events or interactions with other galaxies. The light is fairly uniform with no bright knots of star formation.
