This galaxy appears to be a relatively luminous, elliptical galaxy at a redshift of approximately 0.2. It exhibits a smooth, concentrated light profile, with a slight elongation. The core appears redder in color, potentially indicating an older stellar population or significant dust obscuration in the nucleus. A fainter, extended halo of bluer light surrounds the central region. The lack of distinct spiral arms or other prominent features suggests that the galaxy is likely not undergoing significant star formation currently. There is also a small amount of disturbance on the fringes of the galaxy.
