The galaxy appears to be a relatively luminous, elliptical galaxy, exhibiting a smooth, diffuse structure. The color profile indicates a redder hue in the central region, transitioning to slightly bluer tones towards the outer edges. This may be due to a concentration of older stellar populations and dust in the galactic center, with younger, hotter stars possibly residing in the outskirts, or be the result of redshift. The galaxy's elongated shape suggests it is viewed at an angle. The structure looks largely undisturbed, with no obvious signs of tidal features or significant interactions with other galaxies. There might be some evidence of a slight warp or minor asymmetry in the galaxy's shape, although this is not definitively clear. The galaxy does not appear to be actively forming many new stars.
